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Cassini >> MIMI

CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE
CO-S-MIMI-4-INCA-CALIB-V1.0	PDS 3 CERTIFIED

Start Time: 2004-01-01 16:00:00 - Stop Time: 2017-09-15 03:28:13

This contains calibrated Saturn tour data collected by the INCA sensor of the MIMI instrument aboard the Cassini spacecraft for the Cassini mission.

Citiation Information

Author	Vandegriff J., Kusterer M.B.
Title	CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE
Publisher	NASA Planetary Data System
Publication Year	2018
doi	https://doi.org/10.17189/1519607

Top/ DATA/ IANGAVE0_T/ 2013 /

IANGAVE0_T_2013001_02

Start Time:	2013-001T00:01:17.422	Stop Time:	2013-001T23:57:43.875
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013002_02

Start Time:	2013-002T00:00:40.874	Stop Time:	2013-002T23:57:07.326
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013003_02

Start Time:	2013-003T00:00:03.325	Stop Time:	2013-003T11:24:22.064
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013004_02

Start Time:	2013-004T09:23:23.562	Stop Time:	2013-004T20:33:23.306
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013005_02

Start Time:	2013-005T00:06:24.225	Stop Time:	2013-005T23:58:54.679
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013006_02

Start Time:	2013-006T00:00:24.679	Stop Time:	2013-006T23:58:54.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013007_02

Start Time:	2013-007T00:00:24.130	Stop Time:	2013-007T23:58:39.582
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013008_02

Start Time:	2013-008T00:00:09.581	Stop Time:	2013-008T23:58:39.033
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013009_02

Start Time:	2013-009T00:00:09.033	Stop Time:	2013-009T23:59:25.484
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013010_02

Start Time:	2013-010T00:00:55.484	Stop Time:	2013-010T23:57:55.936
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013011_02

Start Time:	2013-011T01:33:55.900	Stop Time:	2013-011T23:59:23.387
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013012_02

Start Time:	2013-012T00:00:53.386	Stop Time:	2013-012T23:59:22.838
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013013_02

Start Time:	2013-013T00:00:52.837	Stop Time:	2013-013T23:59:23.289
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013014_02

Start Time:	2013-014T00:00:53.289	Stop Time:	2013-014T23:59:23.741
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013015_02

Start Time:	2013-015T00:00:53.740	Stop Time:	2013-015T23:57:38.193
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013016_02

Start Time:	2013-016T00:00:35.191	Stop Time:	2013-016T09:15:45.980
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013017_02

Start Time:	2013-017T04:53:42.531	Stop Time:	2013-017T18:09:47.228
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013018_02

Start Time:	2013-018T03:36:43.012	Stop Time:	2013-018T23:58:43.546
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013019_02

Start Time:	2013-019T00:01:39.545	Stop Time:	2013-019T23:58:31.997
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013020_02

Start Time:	2013-020T00:00:01.997	Stop Time:	2013-020T23:58:31.448
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013021_02

Start Time:	2013-021T00:00:01.448	Stop Time:	2013-021T23:59:19.899
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013022_02

Start Time:	2013-022T00:00:49.899	Stop Time:	2013-022T23:58:48.351
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013023_02

Start Time:	2013-023T00:00:18.350	Stop Time:	2013-023T23:58:47.802
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013024_02

Start Time:	2013-024T00:00:17.802	Stop Time:	2013-024T23:58:48.253
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013025_02

Start Time:	2013-025T00:00:18.253	Stop Time:	2013-025T23:58:48.705
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013026_02

Start Time:	2013-026T00:00:18.704	Stop Time:	2013-026T23:58:48.156
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013027_02

Start Time:	2013-027T00:00:18.155	Stop Time:	2013-027T23:59:03.607
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013028_02

Start Time:	2013-028T00:00:33.607	Stop Time:	2013-028T23:59:49.058
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013029_02

Start Time:	2013-029T00:01:19.058	Stop Time:	2013-029T17:14:23.664
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013030_02

Start Time:	2013-030T14:08:25.186	Stop Time:	2013-030T23:59:00.961
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013031_02

Start Time:	2013-031T00:00:30.960	Stop Time:	2013-031T21:41:30.465
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013032_02

Start Time:	2013-032T01:27:31.378	Stop Time:	2013-032T23:59:00.863
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013033_02

Start Time:	2013-033T00:00:30.863	Stop Time:	2013-033T23:58:30.315
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013034_02

Start Time:	2013-034T00:00:00.314	Stop Time:	2013-034T23:59:29.766
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013035_02

Start Time:	2013-035T00:00:59.765	Stop Time:	2013-035T23:59:29.217
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013036_02

Start Time:	2013-036T00:00:59.216	Stop Time:	2013-036T23:59:29.668
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013037_02

Start Time:	2013-037T00:00:59.668	Stop Time:	2013-037T23:59:30.120
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013038_02

Start Time:	2013-038T00:01:00.119	Stop Time:	2013-038T23:59:29.634
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013039_02

Start Time:	2013-039T00:00:59.634	Stop Time:	2013-039T23:59:30.085
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013040_02

Start Time:	2013-040T00:01:00.084	Stop Time:	2013-040T23:59:30.535
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013041_02

Start Time:	2013-041T00:01:00.535	Stop Time:	2013-041T23:59:29.986
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013042_02

Start Time:	2013-042T00:00:59.985	Stop Time:	2013-042T23:59:30.436
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013043_02

Start Time:	2013-043T00:01:00.436	Stop Time:	2013-043T23:57:41.888
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013044_02

Start Time:	2013-044T00:00:37.886	Stop Time:	2013-044T08:31:45.691
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013045_02

Start Time:	2013-045T05:43:42.206	Stop Time:	2013-045T23:58:35.788
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013046_02

Start Time:	2013-046T00:00:05.788	Stop Time:	2013-046T23:58:35.239
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013047_02

Start Time:	2013-047T00:00:05.238	Stop Time:	2013-047T23:59:20.689
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013048_02

Start Time:	2013-048T00:00:35.688	Stop Time:	2013-048T23:59:06.139
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013049_02

Start Time:	2013-049T00:00:36.139	Stop Time:	2013-049T23:59:06.590
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013050_02

Start Time:	2013-050T00:00:36.589	Stop Time:	2013-050T23:58:53.041
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013051_02

Start Time:	2013-051T00:00:23.040	Stop Time:	2013-051T23:58:10.491
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013052_02

Start Time:	2013-052T00:00:19.490	Stop Time:	2013-052T23:59:27.941
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013053_02

Start Time:	2013-053T00:00:57.941	Stop Time:	2013-053T23:59:34.392
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013054_02

Start Time:	2013-054T00:01:04.391	Stop Time:	2013-054T15:41:24.032
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013055_02

Start Time:	2013-055T05:56:54.706	Stop Time:	2013-055T23:57:52.293
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013056_02

Start Time:	2013-056T00:00:00.293	Stop Time:	2013-056T16:44:05.909
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013057_02

Start Time:	2013-057T01:51:36.700	Stop Time:	2013-057T23:59:06.194
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013058_02

Start Time:	2013-058T00:00:36.193	Stop Time:	2013-058T23:59:06.644
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013059_02

Start Time:	2013-059T00:00:36.644	Stop Time:	2013-059T23:59:07.095
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013060_02

Start Time:	2013-060T00:00:37.094	Stop Time:	2013-060T23:59:06.545
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013061_02

Start Time:	2013-061T00:00:36.545	Stop Time:	2013-061T23:59:06.996
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013062_02

Start Time:	2013-062T00:00:36.995	Stop Time:	2013-062T23:59:07.446
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013063_02

Start Time:	2013-063T00:00:37.446	Stop Time:	2013-063T23:59:06.897
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013064_02

Start Time:	2013-064T00:00:36.896	Stop Time:	2013-064T23:59:07.347
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013065_02

Start Time:	2013-065T00:00:37.347	Stop Time:	2013-065T23:59:06.798
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013066_02

Start Time:	2013-066T00:00:36.797	Stop Time:	2013-066T23:59:07.248
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013067_02

Start Time:	2013-067T00:00:37.248	Stop Time:	2013-067T23:59:07.699
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013068_02

Start Time:	2013-068T00:00:37.698	Stop Time:	2013-068T23:59:53.149
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013069_02

Start Time:	2013-069T00:01:23.148	Stop Time:	2013-069T23:59:53.599
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013070_02

Start Time:	2013-070T00:01:23.599	Stop Time:	2013-070T23:59:53.050
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013071_02

Start Time:	2013-071T00:01:23.049	Stop Time:	2013-071T23:59:51.500
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013072_02

Start Time:	2013-072T00:01:58.500	Stop Time:	2013-072T23:57:58.952
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013073_02

Start Time:	2013-073T00:00:04.951	Stop Time:	2013-073T23:58:45.402
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013074_02

Start Time:	2013-074T00:00:15.401	Stop Time:	2013-074T23:59:53.852
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013075_02

Start Time:	2013-075T00:01:59.851	Stop Time:	2013-075T23:59:15.303
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013076_02

Start Time:	2013-076T00:01:22.302	Stop Time:	2013-076T23:59:35.753
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013077_02

Start Time:	2013-077T00:01:43.752	Stop Time:	2013-077T23:59:01.204
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013078_02

Start Time:	2013-078T00:00:31.203	Stop Time:	2013-078T23:59:12.654
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013079_02

Start Time:	2013-079T00:00:42.654	Stop Time:	2013-079T23:49:18.108
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013080_02

Start Time:	2013-080T00:26:50.094	Stop Time:	2013-080T23:59:49.555
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013081_02

Start Time:	2013-081T00:01:19.554	Stop Time:	2013-081T23:59:58.005
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013082_02

Start Time:	2013-082T00:01:28.005	Stop Time:	2013-082T23:59:30.456
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013083_02

Start Time:	2013-083T00:01:00.455	Stop Time:	2013-083T23:58:55.907
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013084_02

Start Time:	2013-084T00:00:25.906	Stop Time:	2013-084T23:58:56.357
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013085_02

Start Time:	2013-085T00:00:26.357	Stop Time:	2013-085T23:59:26.807
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013086_02

Start Time:	2013-086T00:00:26.807	Stop Time:	2013-086T23:59:28.258
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013087_02

Start Time:	2013-087T00:00:28.258	Stop Time:	2013-087T23:59:33.708
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013088_02

Start Time:	2013-088T00:00:33.708	Stop Time:	2013-088T23:59:11.159
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013089_02

Start Time:	2013-089T00:00:11.159	Stop Time:	2013-089T23:59:27.609
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013090_02

Start Time:	2013-090T00:00:27.609	Stop Time:	2013-090T20:49:46.132
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013091_02

Start Time:	2013-091T10:00:46.830	Stop Time:	2013-091T19:30:46.613
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013092_02

Start Time:	2013-092T12:03:48.234	Stop Time:	2013-092T17:59:18.098
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013093_02

Start Time:	2013-093T02:18:18.908	Stop Time:	2013-093T23:58:48.412
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013094_02

Start Time:	2013-094T00:00:18.411	Stop Time:	2013-094T23:58:48.862
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013095_02

Start Time:	2013-095T00:00:18.861	Stop Time:	2013-095T23:58:49.313
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013096_02

Start Time:	2013-096T00:00:19.312	Stop Time:	2013-096T23:58:28.763
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013097_02

Start Time:	2013-097T00:00:36.762	Stop Time:	2013-097T23:58:01.214
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013098_02

Start Time:	2013-098T00:00:10.213	Stop Time:	2013-098T23:58:56.664
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013099_02

Start Time:	2013-099T00:00:26.663	Stop Time:	2013-099T23:58:57.114
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013100_02

Start Time:	2013-100T00:00:27.114	Stop Time:	2013-100T22:43:57.594
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013101_02

Start Time:	2013-101T01:32:27.529	Stop Time:	2013-101T12:37:27.275
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013102_02

Start Time:	2013-102T01:58:27.970	Stop Time:	2013-102T23:59:58.466
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013103_02

Start Time:	2013-103T00:01:28.465	Stop Time:	2013-103T23:58:39.917
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013104_02

Start Time:	2013-104T00:00:09.916	Stop Time:	2013-104T23:59:26.367
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013105_02

Start Time:	2013-105T00:00:56.366	Stop Time:	2013-105T23:59:25.817
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013106_02

Start Time:	2013-106T00:00:55.817	Stop Time:	2013-106T23:59:26.268
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013107_02

Start Time:	2013-107T00:00:56.267	Stop Time:	2013-107T23:59:57.718
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013108_02

Start Time:	2013-108T00:00:57.718	Stop Time:	2013-108T23:59:59.168
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013109_02

Start Time:	2013-109T00:00:59.168	Stop Time:	2013-109T23:59:29.619
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013110_02

Start Time:	2013-110T00:00:59.619	Stop Time:	2013-110T23:59:30.070
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013111_02

Start Time:	2013-111T00:01:00.069	Stop Time:	2013-111T23:59:00.520
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013112_02

Start Time:	2013-112T00:00:30.520	Stop Time:	2013-112T23:59:00.971
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013113_02

Start Time:	2013-113T00:00:30.970	Stop Time:	2013-113T23:59:40.421
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013114_02

Start Time:	2013-114T00:01:10.420	Stop Time:	2013-114T23:59:40.872
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013115_02

Start Time:	2013-115T00:01:10.871	Stop Time:	2013-115T23:59:41.322
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013116_02

Start Time:	2013-116T00:01:11.321	Stop Time:	2013-116T23:59:40.772
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013117_02

Start Time:	2013-117T00:01:10.772	Stop Time:	2013-117T23:59:02.223
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013118_02

Start Time:	2013-118T00:00:02.223	Stop Time:	2013-118T23:59:10.674
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013119_02

Start Time:	2013-119T00:00:10.673	Stop Time:	2013-119T23:59:21.124
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013120_02

Start Time:	2013-120T00:00:21.124	Stop Time:	2013-120T23:59:50.574
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013121_02

Start Time:	2013-121T00:01:20.574	Stop Time:	2013-121T23:59:21.025
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013122_02

Start Time:	2013-122T00:00:51.024	Stop Time:	2013-122T23:59:40.475
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013123_02

Start Time:	2013-123T00:01:48.475	Stop Time:	2013-123T23:58:48.926
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013124_02

Start Time:	2013-124T00:00:18.926	Stop Time:	2013-124T23:59:53.376
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013125_02

Start Time:	2013-125T00:02:01.376	Stop Time:	2013-125T23:59:22.827
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013126_02

Start Time:	2013-126T00:00:52.826	Stop Time:	2013-126T23:59:23.277
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013127_02

Start Time:	2013-127T00:00:53.277	Stop Time:	2013-127T23:59:23.728
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013128_02

Start Time:	2013-128T00:00:53.727	Stop Time:	2013-128T23:59:23.178
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013129_02

Start Time:	2013-129T00:00:53.178	Stop Time:	2013-129T23:59:23.629
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013130_02

Start Time:	2013-130T00:00:53.628	Stop Time:	2013-130T23:59:24.079
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013131_02

Start Time:	2013-131T00:00:54.079	Stop Time:	2013-131T23:59:24.530
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013132_02

Start Time:	2013-132T00:00:54.529	Stop Time:	2013-132T23:59:52.980
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013133_02

Start Time:	2013-133T00:01:22.980	Stop Time:	2013-133T23:57:58.431
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013134_02

Start Time:	2013-134T00:00:05.431	Stop Time:	2013-134T23:58:43.882
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013135_02

Start Time:	2013-135T00:00:51.881	Stop Time:	2013-135T23:58:40.332
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013136_02

Start Time:	2013-136T00:00:48.331	Stop Time:	2013-136T23:59:06.782
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013137_02

Start Time:	2013-137T00:00:36.782	Stop Time:	2013-137T23:59:19.233
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013138_02

Start Time:	2013-138T00:00:49.232	Stop Time:	2013-138T23:59:19.683
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013139_02

Start Time:	2013-139T00:00:49.683	Stop Time:	2013-139T23:58:55.134
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013140_02

Start Time:	2013-140T00:00:25.133	Stop Time:	2013-140T23:59:56.584
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013141_02

Start Time:	2013-141T00:01:26.584	Stop Time:	2013-141T23:59:57.035
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013142_02

Start Time:	2013-142T00:01:27.034	Stop Time:	2013-142T23:59:56.485
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013143_02

Start Time:	2013-143T00:01:26.485	Stop Time:	2013-143T23:57:56.936
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013144_02

Start Time:	2013-144T00:00:53.935	Stop Time:	2013-144T23:59:58.386
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013145_02

Start Time:	2013-145T00:02:05.385	Stop Time:	2013-145T23:59:48.837
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013146_02

Start Time:	2013-146T00:01:18.836	Stop Time:	2013-146T23:57:26.288
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013147_02

Start Time:	2013-147T00:00:22.287	Stop Time:	2013-147T23:59:44.738
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013148_02

Start Time:	2013-148T00:02:41.736	Stop Time:	2013-148T23:58:41.189
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013149_02

Start Time:	2013-149T00:00:11.188	Stop Time:	2013-149T17:04:11.797
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013150_02

Start Time:	2013-150T04:03:12.546	Stop Time:	2013-150T23:59:43.089
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013151_02

Start Time:	2013-151T00:01:13.089	Stop Time:	2013-151T23:59:43.540
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013152_02

Start Time:	2013-152T00:01:13.539	Stop Time:	2013-152T23:59:43.990
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013153_02

Start Time:	2013-153T00:01:13.990	Stop Time:	2013-153T23:59:28.441
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013154_02

Start Time:	2013-154T00:02:25.440	Stop Time:	2013-154T23:59:49.891
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013155_02

Start Time:	2013-155T00:01:19.890	Stop Time:	2013-155T23:59:13.342
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013156_02

Start Time:	2013-156T00:00:43.341	Stop Time:	2013-156T23:59:07.792
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013157_02

Start Time:	2013-157T00:00:37.792	Stop Time:	2013-157T23:59:07.305
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013158_02

Start Time:	2013-158T00:00:37.305	Stop Time:	2013-158T23:59:07.757
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013159_02

Start Time:	2013-159T00:00:37.756	Stop Time:	2013-159T23:59:28.208
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013160_02

Start Time:	2013-160T00:00:58.207	Stop Time:	2013-160T23:58:41.659
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013161_02

Start Time:	2013-161T00:00:11.659	Stop Time:	2013-161T23:58:50.111
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013162_02

Start Time:	2013-162T00:00:20.110	Stop Time:	2013-162T23:59:55.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013163_02

Start Time:	2013-163T00:01:25.561	Stop Time:	2013-163T23:59:26.013
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013164_02

Start Time:	2013-164T00:00:56.012	Stop Time:	2013-164T23:59:11.464
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013165_02

Start Time:	2013-165T00:01:18.464	Stop Time:	2013-165T23:59:34.915
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013166_02

Start Time:	2013-166T00:01:04.915	Stop Time:	2013-166T23:58:51.367
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013167_02

Start Time:	2013-167T00:00:21.366	Stop Time:	2013-167T23:58:51.818
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013168_02

Start Time:	2013-168T00:00:21.818	Stop Time:	2013-168T23:36:21.278
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013169_02

Start Time:	2013-169T04:42:23.161	Stop Time:	2013-169T23:58:51.721
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013170_02

Start Time:	2013-170T00:00:21.720	Stop Time:	2013-170T23:58:52.172
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013171_02

Start Time:	2013-171T00:00:22.171	Stop Time:	2013-171T23:58:51.623
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013172_02

Start Time:	2013-172T00:00:21.623	Stop Time:	2013-172T23:58:52.075
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013173_02

Start Time:	2013-173T00:00:22.074	Stop Time:	2013-173T15:33:22.718
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013174_02

Start Time:	2013-174T03:36:23.443	Stop Time:	2013-174T13:27:37.218
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013175_02

Start Time:	2013-175T03:43:07.892	Stop Time:	2013-175T23:58:53.428
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013176_02

Start Time:	2013-176T00:00:23.428	Stop Time:	2013-176T23:59:53.879
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013177_02

Start Time:	2013-177T00:01:23.879	Stop Time:	2013-177T23:58:00.331
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013178_02

Start Time:	2013-178T00:00:07.330	Stop Time:	2013-178T23:58:57.782
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013179_02

Start Time:	2013-179T00:01:04.781	Stop Time:	2013-179T23:59:33.233
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013180_02

Start Time:	2013-180T00:01:03.233	Stop Time:	2013-180T23:59:40.684
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013181_02

Start Time:	2013-181T00:01:48.684	Stop Time:	2013-181T23:58:33.136
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013182_02

Start Time:	2013-182T00:00:03.136	Stop Time:	2013-182T23:59:00.587
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013183_02

Start Time:	2013-183T00:00:30.587	Stop Time:	2013-183T23:59:00.039
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013184_02

Start Time:	2013-184T00:00:30.038	Stop Time:	2013-184T23:58:37.490
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013185_02

Start Time:	2013-185T00:00:46.489	Stop Time:	2013-185T23:58:53.941
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013186_02

Start Time:	2013-186T00:00:23.941	Stop Time:	2013-186T23:59:56.392
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013187_02

Start Time:	2013-187T00:01:26.391	Stop Time:	2013-187T23:58:55.844
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013188_02

Start Time:	2013-188T00:00:25.843	Stop Time:	2013-188T23:58:40.295
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013189_02

Start Time:	2013-189T00:00:10.294	Stop Time:	2013-189T23:58:40.746
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013190_02

Start Time:	2013-190T00:00:10.746	Stop Time:	2013-190T23:58:41.198
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013191_02

Start Time:	2013-191T00:00:11.197	Stop Time:	2013-191T23:59:56.648
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013192_02

Start Time:	2013-192T00:01:26.648	Stop Time:	2013-192T23:59:17.100
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013193_02

Start Time:	2013-193T00:00:47.099	Stop Time:	2013-193T23:59:10.551
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013194_02

Start Time:	2013-194T00:00:40.551	Stop Time:	2013-194T23:58:32.003
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013195_02

Start Time:	2013-195T00:00:39.002	Stop Time:	2013-195T23:58:51.454
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013196_02

Start Time:	2013-196T00:01:00.453	Stop Time:	2013-196T23:58:46.905
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013197_02

Start Time:	2013-197T00:00:54.904	Stop Time:	2013-197T23:59:13.356
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013198_02

Start Time:	2013-198T00:01:21.355	Stop Time:	2013-198T23:58:02.808
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013199_02

Start Time:	2013-199T00:00:09.807	Stop Time:	2013-199T23:59:56.258
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013200_02

Start Time:	2013-200T00:02:04.258	Stop Time:	2013-200T21:32:49.766
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013201_02

Start Time:	2013-201T05:56:39.574	Stop Time:	2013-201T21:55:29.208
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013202_02

Start Time:	2013-202T00:36:29.147	Stop Time:	2013-202T23:59:03.613
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013203_02

Start Time:	2013-203T00:00:33.612	Stop Time:	2013-203T23:59:24.064
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013204_02

Start Time:	2013-204T00:00:54.063	Stop Time:	2013-204T23:59:09.515
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013205_02

Start Time:	2013-205T00:00:39.515	Stop Time:	2013-205T23:59:09.966
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013206_02

Start Time:	2013-206T00:00:39.966	Stop Time:	2013-206T23:58:40.418
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013207_02

Start Time:	2013-207T00:00:10.417	Stop Time:	2013-207T23:59:25.869
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013208_02

Start Time:	2013-208T00:00:55.868	Stop Time:	2013-208T23:58:33.320
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013209_02

Start Time:	2013-209T00:00:03.320	Stop Time:	2013-209T23:58:41.772
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013210_02

Start Time:	2013-210T00:00:11.771	Stop Time:	2013-210T23:59:04.223
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013211_02

Start Time:	2013-211T00:00:34.222	Stop Time:	2013-211T23:58:41.674
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013212_02

Start Time:	2013-212T00:00:11.674	Stop Time:	2013-212T23:59:56.125
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013213_02

Start Time:	2013-213T00:01:26.124	Stop Time:	2013-213T23:59:55.576
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013214_02

Start Time:	2013-214T00:01:25.576	Stop Time:	2013-214T23:58:30.028
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013215_02

Start Time:	2013-215T00:00:00.027	Stop Time:	2013-215T23:58:30.479
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013216_02

Start Time:	2013-216T00:00:00.479	Stop Time:	2013-216T23:58:30.931
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013217_02

Start Time:	2013-217T00:00:00.930	Stop Time:	2013-217T23:59:32.381
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013218_02

Start Time:	2013-218T00:01:02.381	Stop Time:	2013-218T10:56:32.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013219_02

Start Time:	2013-219T00:49:32.814	Stop Time:	2013-219T23:59:35.284
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013220_02

Start Time:	2013-220T00:01:05.283	Stop Time:	2013-220T23:59:58.735
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013221_02

Start Time:	2013-221T00:01:28.735	Stop Time:	2013-221T23:59:58.186
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013222_02

Start Time:	2013-222T00:01:28.186	Stop Time:	2013-222T12:14:37.906
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013223_02

Start Time:	2013-223T22:45:35.117	Stop Time:	2013-223T23:59:01.089
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013224_02

Start Time:	2013-224T00:01:57.088	Stop Time:	2013-224T23:58:09.541
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013225_02

Start Time:	2013-225T00:01:05.540	Stop Time:	2013-225T23:57:31.992
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013226_02

Start Time:	2013-226T00:00:28.991	Stop Time:	2013-226T23:59:52.443
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013227_02

Start Time:	2013-227T00:00:52.442	Stop Time:	2013-227T23:59:01.894
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013228_02

Start Time:	2013-228T00:00:01.894	Stop Time:	2013-228T23:59:07.346
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013229_02

Start Time:	2013-229T00:00:37.345	Stop Time:	2013-229T23:59:06.797
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013230_02

Start Time:	2013-230T00:00:36.796	Stop Time:	2013-230T23:59:07.248
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013231_02

Start Time:	2013-231T00:00:37.248	Stop Time:	2013-231T23:59:06.699
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013232_02

Start Time:	2013-232T00:00:36.699	Stop Time:	2013-232T23:59:07.151
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013233_02

Start Time:	2013-233T00:00:37.150	Stop Time:	2013-233T23:59:07.602
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013234_02

Start Time:	2013-234T00:00:37.601	Stop Time:	2013-234T23:59:08.053
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013235_02

Start Time:	2013-235T00:00:08.053	Stop Time:	2013-235T23:59:09.504
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013236_02

Start Time:	2013-236T00:00:09.504	Stop Time:	2013-236T23:59:10.956
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013237_02

Start Time:	2013-237T00:00:10.955	Stop Time:	2013-237T23:59:12.407
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013238_02

Start Time:	2013-238T00:00:12.407	Stop Time:	2013-238T23:59:13.858
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013239_02

Start Time:	2013-239T00:00:13.858	Stop Time:	2013-239T23:59:16.309
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013240_02

Start Time:	2013-240T00:00:16.309	Stop Time:	2013-240T09:34:16.090
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013241_02

Start Time:	2013-241T12:05:48.484	Stop Time:	2013-241T23:59:48.212
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013242_02

Start Time:	2013-242T00:01:18.211	Stop Time:	2013-242T23:59:18.663
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013243_02

Start Time:	2013-243T00:00:33.663	Stop Time:	2013-243T23:58:57.115
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013244_02

Start Time:	2013-244T00:01:05.114	Stop Time:	2013-244T23:59:36.566
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013245_02

Start Time:	2013-245T00:01:06.565	Stop Time:	2013-245T23:59:03.017
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013246_02

Start Time:	2013-246T00:00:33.017	Stop Time:	2013-246T23:59:03.468
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013247_02

Start Time:	2013-247T00:00:33.468	Stop Time:	2013-247T23:59:14.920
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013248_02

Start Time:	2013-248T00:00:44.919	Stop Time:	2013-248T23:59:15.371
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013249_02

Start Time:	2013-249T00:00:45.370	Stop Time:	2013-249T23:59:58.822
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013250_02

Start Time:	2013-250T00:01:28.821	Stop Time:	2013-250T23:59:29.273
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013251_02

Start Time:	2013-251T00:00:29.273	Stop Time:	2013-251T23:59:30.725
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013252_02

Start Time:	2013-252T00:00:30.724	Stop Time:	2013-252T23:59:01.176
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013253_02

Start Time:	2013-253T00:00:31.176	Stop Time:	2013-253T23:59:12.627
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013254_02

Start Time:	2013-254T00:00:42.627	Stop Time:	2013-254T23:59:13.079
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013255_02

Start Time:	2013-255T00:00:43.078	Stop Time:	2013-255T23:58:46.530
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013256_02

Start Time:	2013-256T00:00:53.529	Stop Time:	2013-256T23:59:04.981
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013257_02

Start Time:	2013-257T00:00:04.981	Stop Time:	2013-257T23:59:10.432
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013258_02

Start Time:	2013-258T00:01:18.432	Stop Time:	2013-258T23:59:27.884
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013259_02

Start Time:	2013-259T00:01:34.883	Stop Time:	2013-259T23:58:51.335
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013260_02

Start Time:	2013-260T00:00:21.334	Stop Time:	2013-260T23:58:50.786
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013261_02

Start Time:	2013-261T00:00:20.786	Stop Time:	2013-261T23:58:51.238
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013262_02

Start Time:	2013-262T00:00:21.237	Stop Time:	2013-262T23:59:22.689
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013263_02

Start Time:	2013-263T00:00:22.688	Stop Time:	2013-263T23:59:53.140
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013264_02

Start Time:	2013-264T00:01:08.139	Stop Time:	2013-264T23:59:09.591
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013265_02

Start Time:	2013-265T00:00:09.591	Stop Time:	2013-265T23:59:41.042
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013266_02

Start Time:	2013-266T00:00:56.042	Stop Time:	2013-266T23:59:10.494
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013267_02

Start Time:	2013-267T00:00:40.493	Stop Time:	2013-267T23:59:10.945
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013268_02

Start Time:	2013-268T00:00:40.944	Stop Time:	2013-268T23:59:11.396
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013269_02

Start Time:	2013-269T00:00:41.396	Stop Time:	2013-269T23:59:10.848
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013270_02

Start Time:	2013-270T00:00:40.847	Stop Time:	2013-270T23:59:41.299
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013271_02

Start Time:	2013-271T00:01:11.298	Stop Time:	2013-271T23:59:41.750
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013272_02

Start Time:	2013-272T00:01:11.749	Stop Time:	2013-272T23:58:12.202
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013273_02

Start Time:	2013-273T00:00:19.201	Stop Time:	2013-273T23:59:51.652
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013274_02

Start Time:	2013-274T00:04:07.651	Stop Time:	2013-274T07:04:48.490
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013275_02

Start Time:	2013-275T20:13:20.641	Stop Time:	2013-275T23:59:21.555
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013276_02

Start Time:	2013-276T00:01:28.554	Stop Time:	2013-276T23:59:07.007
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013277_02

Start Time:	2013-277T00:00:37.006	Stop Time:	2013-277T23:59:08.458
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013278_02

Start Time:	2013-278T00:01:15.457	Stop Time:	2013-278T23:59:56.909
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013279_02

Start Time:	2013-279T00:01:26.908	Stop Time:	2013-279T23:59:11.360
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013280_02

Start Time:	2013-280T00:00:41.360	Stop Time:	2013-280T23:59:52.811
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013281_02

Start Time:	2013-281T00:01:22.811	Stop Time:	2013-281T23:59:52.263
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013282_02

Start Time:	2013-282T00:01:22.262	Stop Time:	2013-282T23:59:52.714
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013283_02

Start Time:	2013-283T00:01:22.713	Stop Time:	2013-283T23:59:53.165
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013284_02

Start Time:	2013-284T00:01:23.165	Stop Time:	2013-284T23:59:52.616
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013285_02

Start Time:	2013-285T00:01:22.616	Stop Time:	2013-285T23:59:53.068
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013286_02

Start Time:	2013-286T00:01:23.067	Stop Time:	2013-286T23:12:23.537
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013287_02

Start Time:	2013-287T00:50:23.500	Stop Time:	2013-287T23:59:13.970
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013288_02

Start Time:	2013-288T00:01:21.970	Stop Time:	2013-288T23:58:33.422
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013289_02

Start Time:	2013-289T00:00:03.421	Stop Time:	2013-289T23:58:52.873
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013290_02

Start Time:	2013-290T00:00:22.873	Stop Time:	2013-290T23:59:56.324
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013291_02

Start Time:	2013-291T00:01:26.323	Stop Time:	2013-291T23:59:21.775
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013292_02

Start Time:	2013-292T00:00:51.775	Stop Time:	2013-292T23:59:22.227
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013293_02

Start Time:	2013-293T00:00:52.226	Stop Time:	2013-293T23:59:56.678
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013294_02

Start Time:	2013-294T00:00:56.677	Stop Time:	2013-294T23:59:57.129
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013295_02

Start Time:	2013-295T00:01:27.128	Stop Time:	2013-295T23:59:57.580
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013296_02

Start Time:	2013-296T00:01:27.580	Stop Time:	2013-296T23:59:58.032
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013297_02

Start Time:	2013-297T00:01:28.031	Stop Time:	2013-297T23:59:57.483
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013298_02

Start Time:	2013-298T00:01:27.482	Stop Time:	2013-298T23:59:57.934
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013299_02

Start Time:	2013-299T00:01:27.934	Stop Time:	2013-299T23:59:58.385
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013300_02

Start Time:	2013-300T00:01:28.385	Stop Time:	2013-300T23:59:57.837
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013301_02

Start Time:	2013-301T00:01:27.836	Stop Time:	2013-301T23:59:58.288
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013302_02

Start Time:	2013-302T00:01:28.287	Stop Time:	2013-302T23:59:58.739
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013303_02

Start Time:	2013-303T00:01:28.739	Stop Time:	2013-303T23:58:44.191
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013304_02

Start Time:	2013-304T00:00:14.190	Stop Time:	2013-304T23:58:43.642
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013305_02

Start Time:	2013-305T00:03:13.640	Stop Time:	2013-305T23:58:44.093
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013306_02

Start Time:	2013-306T00:00:14.093	Stop Time:	2013-306T23:58:44.545
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013307_02

Start Time:	2013-307T00:00:14.544	Stop Time:	2013-307T23:59:43.996
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013308_02

Start Time:	2013-308T00:02:43.994	Stop Time:	2013-308T23:59:44.447
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013309_02

Start Time:	2013-309T00:01:14.446	Stop Time:	2013-309T17:16:14.052
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013310_02

Start Time:	2013-310T13:44:43.584	Stop Time:	2013-310T23:59:44.349
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013311_02

Start Time:	2013-311T00:01:14.349	Stop Time:	2013-311T23:47:45.805
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013312_02

Start Time:	2013-312T00:04:13.799	Stop Time:	2013-312T23:59:44.252
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013313_02

Start Time:	2013-313T00:01:14.251	Stop Time:	2013-313T11:29:43.989
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013314_02

Start Time:	2013-314T09:20:45.489	Stop Time:	2013-314T23:59:43.155
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013315_02

Start Time:	2013-315T00:13:15.149	Stop Time:	2013-315T04:29:44.052
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013316_02

Start Time:	2013-316T10:12:46.372	Stop Time:	2013-316T23:59:46.057
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013317_02

Start Time:	2013-317T00:01:16.056	Stop Time:	2013-317T23:59:46.508
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013318_02

Start Time:	2013-318T00:01:16.508	Stop Time:	2013-318T23:59:46.960
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013319_02

Start Time:	2013-319T00:01:16.959	Stop Time:	2013-319T23:59:16.411
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013320_02

Start Time:	2013-320T00:00:46.410	Stop Time:	2013-320T23:59:16.862
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013321_02

Start Time:	2013-321T00:00:46.862	Stop Time:	2013-321T23:59:17.314
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013322_02

Start Time:	2013-322T00:00:47.313	Stop Time:	2013-322T23:59:30.765
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013323_02

Start Time:	2013-323T00:01:00.764	Stop Time:	2013-323T23:59:31.216
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013324_02

Start Time:	2013-324T00:01:01.215	Stop Time:	2013-324T23:59:51.667
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013325_02

Start Time:	2013-325T00:01:21.667	Stop Time:	2013-325T23:59:56.118
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013326_02

Start Time:	2013-326T00:01:26.118	Stop Time:	2013-326T23:58:34.570
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013327_02

Start Time:	2013-327T00:00:04.570	Stop Time:	2013-327T23:59:51.021
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013328_02

Start Time:	2013-328T00:01:21.020	Stop Time:	2013-328T23:59:00.473
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013329_02

Start Time:	2013-329T00:00:30.472	Stop Time:	2013-329T23:59:11.924
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013330_02

Start Time:	2013-330T00:00:41.923	Stop Time:	2013-330T23:58:51.375
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013331_02

Start Time:	2013-331T00:00:21.375	Stop Time:	2013-331T23:58:32.827
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013332_02

Start Time:	2013-332T00:00:02.826	Stop Time:	2013-332T23:58:56.278
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013333_02

Start Time:	2013-333T00:01:03.277	Stop Time:	2013-333T23:59:05.729
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013334_02

Start Time:	2013-334T00:00:35.728	Stop Time:	2013-334T23:59:36.180
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013335_02

Start Time:	2013-335T00:00:21.180	Stop Time:	2013-335T23:59:47.631
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013336_02

Start Time:	2013-336T00:01:54.630	Stop Time:	2013-336T23:58:42.083
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013337_02

Start Time:	2013-337T00:00:12.082	Stop Time:	2013-337T23:59:54.534
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013338_02

Start Time:	2013-338T00:01:24.533	Stop Time:	2013-338T23:59:52.985
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013339_02

Start Time:	2013-339T00:01:22.984	Stop Time:	2013-339T21:41:47.489
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013340_02

Start Time:	2013-340T09:27:48.220	Stop Time:	2013-340T12:12:18.157
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013341_02

Start Time:	2013-341T09:33:19.669	Stop Time:	2013-341T23:59:50.339
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013342_02

Start Time:	2013-342T00:01:20.338	Stop Time:	2013-342T23:59:49.790
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013343_02

Start Time:	2013-343T00:01:19.789	Stop Time:	2013-343T23:59:50.241
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013344_02

Start Time:	2013-344T00:01:20.241	Stop Time:	2013-344T23:59:50.693
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013345_02

Start Time:	2013-345T00:01:20.692	Stop Time:	2013-345T23:59:50.144
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013346_02

Start Time:	2013-346T00:01:20.143	Stop Time:	2013-346T23:59:50.595
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013347_02

Start Time:	2013-347T00:01:20.595	Stop Time:	2013-347T23:59:50.046
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013348_02

Start Time:	2013-348T00:01:20.046	Stop Time:	2013-348T23:59:50.498
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013349_02

Start Time:	2013-349T00:01:20.497	Stop Time:	2013-349T23:59:50.949
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013350_02

Start Time:	2013-350T00:01:20.948	Stop Time:	2013-350T23:59:50.400
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013351_02

Start Time:	2013-351T00:01:20.400	Stop Time:	2013-351T23:58:35.852
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013352_02

Start Time:	2013-352T00:00:05.851	Stop Time:	2013-352T23:58:17.303
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013353_02

Start Time:	2013-353T00:00:27.302	Stop Time:	2013-353T23:59:55.754
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013354_02

Start Time:	2013-354T00:01:25.753	Stop Time:	2013-354T23:58:35.206
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013355_02

Start Time:	2013-355T00:00:05.205	Stop Time:	2013-355T23:58:35.657
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013356_02

Start Time:	2013-356T00:00:05.656	Stop Time:	2013-356T23:58:36.108
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013357_02

Start Time:	2013-357T00:00:06.108	Stop Time:	2013-357T23:58:35.560
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013358_02

Start Time:	2013-358T00:00:05.559	Stop Time:	2013-358T23:58:36.011
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013359_02

Start Time:	2013-359T00:00:06.010	Stop Time:	2013-359T23:58:36.462
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013360_02

Start Time:	2013-360T00:00:06.461	Stop Time:	2013-360T23:58:35.913
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013361_02

Start Time:	2013-361T00:00:05.913	Stop Time:	2013-361T23:58:36.287
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013362_02

Start Time:	2013-362T00:00:06.286	Stop Time:	2013-362T23:59:08.738
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013363_02

Start Time:	2013-363T00:01:14.737	Stop Time:	2013-363T23:58:37.189
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013364_02

Start Time:	2013-364T00:00:07.188	Stop Time:	2013-364T23:59:20.639
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2013365_02

Start Time:	2013-365T00:01:27.638	Stop Time:	2013-365T23:59:02.090
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

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