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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

CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE

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/ 2010 /

IANGAVE0_T_2010001_02

Start Time:	2010-001T00:00:13.883	Stop Time:	2010-001T23:59:45.268
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_2010002_02

Start Time:	2010-002T00:00:45.268	Stop Time:	2010-002T23:59:30.654
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_2010003_02

Start Time:	2010-003T00:00:30.654	Stop Time:	2010-003T23:59:32.040
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010004_02

Start Time:	2010-004T00:00:32.039	Stop Time:	2010-004T23:59:33.425
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010005_02

Start Time:	2010-005T00:00:33.425	Stop Time:	2010-005T19:34:02.924
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_2010006_02

Start Time:	2010-006T01:44:42.766	Stop Time:	2010-006T15:31:41.413
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010007_02

Start Time:	2010-007T04:50:43.072	Stop Time:	2010-007T20:20:50.675
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010008_02

Start Time:	2010-008T00:08:51.578	Stop Time:	2010-008T23:59:16.968
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010009_02

Start Time:	2010-009T00:00:16.967	Stop Time:	2010-009T22:02:21.403
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010010_02

Start Time:	2010-010T00:03:06.352	Stop Time:	2010-010T23:59:25.739
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_2010011_02

Start Time:	2010-011T00:00:40.738	Stop Time:	2010-011T09:56:56.458
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_2010012_02

Start Time:	2010-012T05:59:55.942	Stop Time:	2010-012T23:59:56.479
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_2010013_02

Start Time:	2010-013T00:00:41.478	Stop Time:	2010-013T23:58:42.862
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_2010014_02

Start Time:	2010-014T00:00:12.861	Stop Time:	2010-014T23:58:15.245
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010015_02

Start Time:	2010-015T00:00:23.244	Stop Time:	2010-015T23:58:48.627
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_2010016_02

Start Time:	2010-016T00:00:58.626	Stop Time:	2010-016T23:58:32.010
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010017_02

Start Time:	2010-017T00:00:40.009	Stop Time:	2010-017T23:58:18.392
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_2010018_02

Start Time:	2010-018T00:00:27.391	Stop Time:	2010-018T23:57:58.775
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_2010019_02

Start Time:	2010-019T00:00:05.774	Stop Time:	2010-019T23:59:46.157
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_2010020_02

Start Time:	2010-020T00:01:54.156	Stop Time:	2010-020T23:59:55.539
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010021_02

Start Time:	2010-021T00:02:04.539	Stop Time:	2010-021T23:59:05.922
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010022_02

Start Time:	2010-022T00:01:14.921	Stop Time:	2010-022T23:59:41.305
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_2010023_02

Start Time:	2010-023T00:00:41.304	Stop Time:	2010-023T23:59:12.688
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010024_02

Start Time:	2010-024T00:00:12.687	Stop Time:	2010-024T23:59:07.070
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_2010025_02

Start Time:	2010-025T00:00:07.070	Stop Time:	2010-025T23:58:29.492
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010026_02

Start Time:	2010-026T00:00:35.491	Stop Time:	2010-026T20:30:26.966
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_2010027_02

Start Time:	2010-027T05:19:57.740	Stop Time:	2010-027T23:59:22.262
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010028_02

Start Time:	2010-028T00:01:30.261	Stop Time:	2010-028T23:59:12.647
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010029_02

Start Time:	2010-029T00:00:12.647	Stop Time:	2010-029T23:59:14.033
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_2010030_02

Start Time:	2010-030T00:00:14.032	Stop Time:	2010-030T23:58:02.418
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_2010031_02

Start Time:	2010-031T00:00:09.417	Stop Time:	2010-031T23:59:21.803
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010032_02

Start Time:	2010-032T00:01:28.802	Stop Time:	2010-032T23:59:45.188
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010033_02

Start Time:	2010-033T00:00:45.187	Stop Time:	2010-033T23:59:31.573
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010034_02

Start Time:	2010-034T00:00:31.573	Stop Time:	2010-034T23:59:15.958
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010035_02

Start Time:	2010-035T00:00:15.958	Stop Time:	2010-035T23:59:47.343
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010036_02

Start Time:	2010-036T00:00:47.343	Stop Time:	2010-036T23:59:48.728
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_2010037_02

Start Time:	2010-037T00:00:48.728	Stop Time:	2010-037T23:59:50.114
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_2010038_02

Start Time:	2010-038T00:00:50.113	Stop Time:	2010-038T23:59:40.499
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010039_02

Start Time:	2010-039T00:00:55.498	Stop Time:	2010-039T23:59:51.884
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_2010040_02

Start Time:	2010-040T00:01:06.883	Stop Time:	2010-040T23:58:05.270
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010041_02

Start Time:	2010-041T00:00:12.269	Stop Time:	2010-041T23:58:42.655
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010042_02

Start Time:	2010-042T00:00:49.654	Stop Time:	2010-042T23:59:53.039
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_2010043_02

Start Time:	2010-043T00:02:01.039	Stop Time:	2010-043T23:59:04.425
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010044_02

Start Time:	2010-044T00:00:19.424	Stop Time:	2010-044T23:59:20.810
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010045_02

Start Time:	2010-045T00:00:35.809	Stop Time:	2010-045T23:58:38.195
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010046_02

Start Time:	2010-046T00:00:46.195	Stop Time:	2010-046T23:59:20.580
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_2010047_02

Start Time:	2010-047T00:00:35.580	Stop Time:	2010-047T23:59:27.965
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010048_02

Start Time:	2010-048T00:01:36.965	Stop Time:	2010-048T23:59:48.350
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010049_02

Start Time:	2010-049T00:01:03.350	Stop Time:	2010-049T23:59:04.736
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010050_02

Start Time:	2010-050T00:00:04.735	Stop Time:	2010-050T23:59:06.121
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010051_02

Start Time:	2010-051T00:00:06.121	Stop Time:	2010-051T23:58:52.506
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010052_02

Start Time:	2010-052T00:01:01.505	Stop Time:	2010-052T23:59:14.891
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_2010053_02

Start Time:	2010-053T00:00:14.891	Stop Time:	2010-053T23:59:16.276
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010054_02

Start Time:	2010-054T00:00:16.276	Stop Time:	2010-054T23:59:13.662
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010055_02

Start Time:	2010-055T00:00:28.661	Stop Time:	2010-055T23:59:11.047
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010056_02

Start Time:	2010-056T00:00:11.046	Stop Time:	2010-056T23:59:03.432
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_2010057_02

Start Time:	2010-057T00:00:18.432	Stop Time:	2010-057T23:59:12.817
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_2010058_02

Start Time:	2010-058T00:00:27.817	Stop Time:	2010-058T23:59:14.202
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_2010059_02

Start Time:	2010-059T00:00:14.202	Stop Time:	2010-059T23:59:00.588
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010060_02

Start Time:	2010-060T00:00:00.587	Stop Time:	2010-060T23:59:01.973
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010061_02

Start Time:	2010-061T00:00:01.972	Stop Time:	2010-061T23:59:46.358
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010062_02

Start Time:	2010-062T00:00:46.357	Stop Time:	2010-062T23:59:41.743
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010063_02

Start Time:	2010-063T00:00:41.742	Stop Time:	2010-063T23:59:02.091
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010064_02

Start Time:	2010-064T00:01:11.090	Stop Time:	2010-064T23:58:59.475
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_2010065_02

Start Time:	2010-065T00:00:14.474	Stop Time:	2010-065T23:57:05.859
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010066_02

Start Time:	2010-066T00:01:06.857	Stop Time:	2010-066T23:58:59.241
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_2010067_02

Start Time:	2010-067T00:00:14.241	Stop Time:	2010-067T23:58:36.625
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010068_02

Start Time:	2010-068T00:00:44.624	Stop Time:	2010-068T23:59:57.008
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010069_02

Start Time:	2010-069T00:02:04.007	Stop Time:	2010-069T23:59:49.391
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010070_02

Start Time:	2010-070T00:00:49.391	Stop Time:	2010-070T23:58:48.775
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_2010071_02

Start Time:	2010-071T00:00:03.775	Stop Time:	2010-071T23:59:20.158
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010072_02

Start Time:	2010-072T00:00:20.158	Stop Time:	2010-072T23:59:01.542
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010073_02

Start Time:	2010-073T00:00:01.542	Stop Time:	2010-073T23:58:47.926
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_2010074_02

Start Time:	2010-074T00:00:02.925	Stop Time:	2010-074T23:59:49.309
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_2010075_02

Start Time:	2010-075T00:00:49.308	Stop Time:	2010-075T23:59:33.692
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010076_02

Start Time:	2010-076T00:00:33.692	Stop Time:	2010-076T23:58:34.100
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_2010077_02

Start Time:	2010-077T00:00:43.099	Stop Time:	2010-077T23:58:48.489
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_2010078_02

Start Time:	2010-078T00:00:56.488	Stop Time:	2010-078T23:59:53.877
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010079_02

Start Time:	2010-079T00:00:53.877	Stop Time:	2010-079T23:59:39.266
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010080_02

Start Time:	2010-080T00:00:54.266	Stop Time:	2010-080T23:59:40.655
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010081_02

Start Time:	2010-081T00:00:55.654	Stop Time:	2010-081T15:22:13.263
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_2010082_02

Start Time:	2010-082T22:58:51.458	Stop Time:	2010-082T23:59:12.432
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_2010083_02

Start Time:	2010-083T00:00:59.432	Stop Time:	2010-083T23:58:42.821
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010084_02

Start Time:	2010-084T00:00:12.821	Stop Time:	2010-084T23:58:43.210
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010085_02

Start Time:	2010-085T00:00:13.209	Stop Time:	2010-085T23:59:48.598
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010086_02

Start Time:	2010-086T00:01:18.598	Stop Time:	2010-086T23:59:25.987
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010087_02

Start Time:	2010-087T00:02:25.986	Stop Time:	2010-087T23:59:27.376
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_2010088_02

Start Time:	2010-088T00:00:27.376	Stop Time:	2010-088T23:59:10.765
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_2010089_02

Start Time:	2010-089T00:00:10.764	Stop Time:	2010-089T23:59:55.129
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_2010090_02

Start Time:	2010-090T00:00:55.129	Stop Time:	2010-090T23:59:56.514
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010091_02

Start Time:	2010-091T00:00:56.514	Stop Time:	2010-091T23:59:14.900
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010092_02

Start Time:	2010-092T00:00:14.899	Stop Time:	2010-092T23:59:45.284
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_2010093_02

Start Time:	2010-093T00:00:45.284	Stop Time:	2010-093T23:59:32.670
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010094_02

Start Time:	2010-094T00:00:32.669	Stop Time:	2010-094T23:59:37.055
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010095_02

Start Time:	2010-095T00:00:37.054	Stop Time:	2010-095T23:59:53.440
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010096_02

Start Time:	2010-096T00:00:53.439	Stop Time:	2010-096T22:04:09.874
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010097_02

Start Time:	2010-097T04:47:01.515	Stop Time:	2010-097T23:59:26.210
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010098_02

Start Time:	2010-098T00:00:41.210	Stop Time:	2010-098T23:59:24.595
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_2010099_02

Start Time:	2010-099T00:00:39.595	Stop Time:	2010-099T23:59:28.980
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_2010100_02

Start Time:	2010-100T00:00:44.980	Stop Time:	2010-100T23:59:27.365
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010101_02

Start Time:	2010-101T00:00:27.365	Stop Time:	2010-101T23:59:57.750
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_2010102_02

Start Time:	2010-102T00:00:57.750	Stop Time:	2010-102T23:59:28.136
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_2010103_02

Start Time:	2010-103T00:00:43.135	Stop Time:	2010-103T23:59:33.521
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010104_02

Start Time:	2010-104T00:00:33.520	Stop Time:	2010-104T23:59:35.906
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_2010105_02

Start Time:	2010-105T00:00:50.905	Stop Time:	2010-105T23:59:21.291
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010106_02

Start Time:	2010-106T00:00:21.290	Stop Time:	2010-106T23:59:29.629
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_2010107_02

Start Time:	2010-107T00:00:29.628	Stop Time:	2010-107T19:15:45.133
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010108_02

Start Time:	2010-108T06:33:30.843	Stop Time:	2010-108T13:21:00.668
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_2010109_02

Start Time:	2010-109T15:32:30.994	Stop Time:	2010-109T23:59:31.777
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010110_02

Start Time:	2010-110T00:00:31.777	Stop Time:	2010-110T23:59:18.160
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010111_02

Start Time:	2010-111T00:00:18.160	Stop Time:	2010-111T23:59:01.543
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010112_02

Start Time:	2010-112T00:00:01.543	Stop Time:	2010-112T23:59:31.926
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_2010113_02

Start Time:	2010-113T00:00:31.925	Stop Time:	2010-113T23:59:33.309
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_2010114_02

Start Time:	2010-114T00:00:33.308	Stop Time:	2010-114T23:59:49.691
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_2010115_02

Start Time:	2010-115T00:00:49.691	Stop Time:	2010-115T23:59:36.074
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010116_02

Start Time:	2010-116T00:00:36.074	Stop Time:	2010-116T23:59:21.457
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010117_02

Start Time:	2010-117T00:00:36.457	Stop Time:	2010-117T23:59:51.840
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010118_02

Start Time:	2010-118T00:00:36.839	Stop Time:	2010-118T23:59:24.223
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_2010119_02

Start Time:	2010-119T00:00:39.222	Stop Time:	2010-119T23:59:05.606
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010120_02

Start Time:	2010-120T00:00:05.605	Stop Time:	2010-120T23:59:51.988
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010121_02

Start Time:	2010-121T00:01:06.988	Stop Time:	2010-121T23:59:22.371
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_2010122_02

Start Time:	2010-122T00:00:37.371	Stop Time:	2010-122T23:59:38.754
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_2010123_02

Start Time:	2010-123T00:00:53.754	Stop Time:	2010-123T23:59:25.137
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010124_02

Start Time:	2010-124T00:00:25.137	Stop Time:	2010-124T23:59:25.520
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_2010125_02

Start Time:	2010-125T00:00:40.519	Stop Time:	2010-125T23:58:56.903
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010126_02

Start Time:	2010-126T00:00:11.902	Stop Time:	2010-126T23:59:43.285
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010127_02

Start Time:	2010-127T00:00:58.285	Stop Time:	2010-127T23:59:13.668
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_2010128_02

Start Time:	2010-128T00:00:13.668	Stop Time:	2010-128T23:58:45.052
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_2010129_02

Start Time:	2010-129T00:00:00.051	Stop Time:	2010-129T23:59:01.434
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010130_02

Start Time:	2010-130T00:00:16.434	Stop Time:	2010-130T23:59:02.817
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_2010131_02

Start Time:	2010-131T00:00:17.817	Stop Time:	2010-131T23:59:49.200
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010132_02

Start Time:	2010-132T00:00:49.199	Stop Time:	2010-132T23:59:34.583
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010133_02

Start Time:	2010-133T00:00:34.582	Stop Time:	2010-133T23:59:10.966
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_2010134_02

Start Time:	2010-134T00:01:18.965	Stop Time:	2010-134T23:59:25.348
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010135_02

Start Time:	2010-135T00:01:31.347	Stop Time:	2010-135T23:58:41.731
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010136_02

Start Time:	2010-136T00:00:49.731	Stop Time:	2010-136T23:59:03.114
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_2010137_02

Start Time:	2010-137T00:00:03.114	Stop Time:	2010-137T23:59:50.497
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010138_02

Start Time:	2010-138T00:00:50.496	Stop Time:	2010-138T23:59:06.880
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010139_02

Start Time:	2010-139T00:00:21.879	Stop Time:	2010-139T23:59:22.263
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_2010140_02

Start Time:	2010-140T00:00:52.262	Stop Time:	2010-140T23:59:22.645
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010141_02

Start Time:	2010-141T00:00:52.645	Stop Time:	2010-141T22:02:53.078
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010142_02

Start Time:	2010-142T02:09:52.972	Stop Time:	2010-142T23:59:11.411
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_2010143_02

Start Time:	2010-143T00:00:11.411	Stop Time:	2010-143T23:59:39.794
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010144_02

Start Time:	2010-144T00:00:39.793	Stop Time:	2010-144T23:58:27.177
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010145_02

Start Time:	2010-145T00:00:27.176	Stop Time:	2010-145T23:59:28.560
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_2010146_02

Start Time:	2010-146T00:00:28.559	Stop Time:	2010-146T23:59:29.942
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010147_02

Start Time:	2010-147T00:00:29.942	Stop Time:	2010-147T23:59:31.325
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010148_02

Start Time:	2010-148T00:00:31.325	Stop Time:	2010-148T23:59:16.708
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_2010149_02

Start Time:	2010-149T00:00:16.708	Stop Time:	2010-149T23:59:50.091
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010150_02

Start Time:	2010-150T00:01:20.090	Stop Time:	2010-150T23:58:49.474
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010151_02

Start Time:	2010-151T00:00:19.473	Stop Time:	2010-151T23:59:07.857
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010152_02

Start Time:	2010-152T00:00:37.856	Stop Time:	2010-152T23:58:45.259
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010153_02

Start Time:	2010-153T00:00:15.258	Stop Time:	2010-153T23:03:13.665
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010154_02

Start Time:	2010-154T07:58:14.436	Stop Time:	2010-154T23:59:44.024
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010155_02

Start Time:	2010-155T00:01:14.023	Stop Time:	2010-155T23:59:32.407
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_2010156_02

Start Time:	2010-156T00:01:02.406	Stop Time:	2010-156T23:59:32.790
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_2010157_02

Start Time:	2010-157T00:01:02.789	Stop Time:	2010-157T23:59:25.172
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_2010158_02

Start Time:	2010-158T00:01:32.172	Stop Time:	2010-158T23:59:18.555
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_2010159_02

Start Time:	2010-159T00:01:26.554	Stop Time:	2010-159T23:58:33.938
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010160_02

Start Time:	2010-160T00:00:42.937	Stop Time:	2010-160T23:59:45.321
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010161_02

Start Time:	2010-161T00:01:54.320	Stop Time:	2010-161T23:59:04.704
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010162_02

Start Time:	2010-162T00:00:04.703	Stop Time:	2010-162T23:59:05.086
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010163_02

Start Time:	2010-163T00:00:05.086	Stop Time:	2010-163T23:59:03.469
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010164_02

Start Time:	2010-164T00:00:03.469	Stop Time:	2010-164T23:59:40.852
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_2010165_02

Start Time:	2010-165T00:00:40.851	Stop Time:	2010-165T23:59:07.235
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010166_02

Start Time:	2010-166T00:00:07.234	Stop Time:	2010-166T23:58:25.618
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010167_02

Start Time:	2010-167T00:00:33.617	Stop Time:	2010-167T23:59:13.000
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010168_02

Start Time:	2010-168T00:01:21.999	Stop Time:	2010-168T23:59:23.383
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010169_02

Start Time:	2010-169T00:00:38.382	Stop Time:	2010-169T23:59:58.765
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_2010170_02

Start Time:	2010-170T00:01:13.765	Stop Time:	2010-170T23:59:00.149
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_2010171_02

Start Time:	2010-171T00:00:15.148	Stop Time:	2010-171T23:59:34.531
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010172_02

Start Time:	2010-172T00:00:34.531	Stop Time:	2010-172T23:59:50.914
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010173_02

Start Time:	2010-173T00:00:50.913	Stop Time:	2010-173T23:59:09.297
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010174_02

Start Time:	2010-174T00:01:17.296	Stop Time:	2010-174T23:59:44.679
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_2010175_02

Start Time:	2010-175T00:00:44.679	Stop Time:	2010-175T23:59:23.062
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010176_02

Start Time:	2010-176T00:00:23.062	Stop Time:	2010-176T23:58:57.445
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010177_02

Start Time:	2010-177T00:00:12.445	Stop Time:	2010-177T23:59:54.828
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010178_02

Start Time:	2010-178T00:02:02.827	Stop Time:	2010-178T23:59:03.211
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010179_02

Start Time:	2010-179T00:01:11.210	Stop Time:	2010-179T23:58:58.594
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_2010180_02

Start Time:	2010-180T00:00:13.593	Stop Time:	2010-180T23:59:58.976
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010181_02

Start Time:	2010-181T00:01:13.975	Stop Time:	2010-181T23:59:23.331
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_2010182_02

Start Time:	2010-182T00:00:38.331	Stop Time:	2010-182T23:58:45.711
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010183_02

Start Time:	2010-183T00:00:00.710	Stop Time:	2010-183T23:59:46.090
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_2010184_02

Start Time:	2010-184T00:01:16.089	Stop Time:	2010-184T23:58:46.470
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010185_02

Start Time:	2010-185T00:00:16.469	Stop Time:	2010-185T20:32:46.938
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010186_02

Start Time:	2010-186T03:36:46.755	Stop Time:	2010-186T23:59:17.228
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_2010187_02

Start Time:	2010-187T00:00:47.227	Stop Time:	2010-187T23:59:47.607
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_2010188_02

Start Time:	2010-188T00:00:32.607	Stop Time:	2010-188T19:31:49.102
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010189_02

Start Time:	2010-189T01:10:48.956	Stop Time:	2010-189T23:59:19.366
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010190_02

Start Time:	2010-190T00:00:49.366	Stop Time:	2010-190T23:59:33.746
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_2010191_02

Start Time:	2010-191T00:01:03.745	Stop Time:	2010-191T23:59:07.125
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_2010192_02

Start Time:	2010-192T00:00:37.124	Stop Time:	2010-192T23:58:42.505
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010193_02

Start Time:	2010-193T00:00:12.504	Stop Time:	2010-193T23:59:00.884
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_2010194_02

Start Time:	2010-194T00:00:30.883	Stop Time:	2010-194T23:58:33.264
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010195_02

Start Time:	2010-195T00:00:03.263	Stop Time:	2010-195T23:58:40.643
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010196_02

Start Time:	2010-196T00:00:10.642	Stop Time:	2010-196T23:58:41.022
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010197_02

Start Time:	2010-197T00:00:11.022	Stop Time:	2010-197T23:59:03.401
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010198_02

Start Time:	2010-198T00:00:33.401	Stop Time:	2010-198T23:59:53.780
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010199_02

Start Time:	2010-199T00:01:23.780	Stop Time:	2010-199T23:59:25.160
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010200_02

Start Time:	2010-200T00:00:55.159	Stop Time:	2010-200T23:58:48.540
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_2010201_02

Start Time:	2010-201T00:00:18.539	Stop Time:	2010-201T23:58:48.919
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010202_02

Start Time:	2010-202T00:00:18.918	Stop Time:	2010-202T23:59:29.298
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010203_02

Start Time:	2010-203T00:00:59.298	Stop Time:	2010-203T23:59:59.677
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010204_02

Start Time:	2010-204T00:01:29.677	Stop Time:	2010-204T23:59:12.057
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_2010205_02

Start Time:	2010-205T00:00:42.056	Stop Time:	2010-205T23:59:12.436
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_2010206_02

Start Time:	2010-206T00:00:42.436	Stop Time:	2010-206T23:59:12.816
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010207_02

Start Time:	2010-207T00:00:42.815	Stop Time:	2010-207T23:59:14.195
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010208_02

Start Time:	2010-208T00:00:14.195	Stop Time:	2010-208T23:59:17.575
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010209_02

Start Time:	2010-209T00:00:17.574	Stop Time:	2010-209T23:59:14.954
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010210_02

Start Time:	2010-210T00:00:14.954	Stop Time:	2010-210T23:59:02.333
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010211_02

Start Time:	2010-211T00:00:02.333	Stop Time:	2010-211T23:59:04.713
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010212_02

Start Time:	2010-212T00:00:04.712	Stop Time:	2010-212T23:59:52.092
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010213_02

Start Time:	2010-213T00:00:52.091	Stop Time:	2010-213T23:59:56.471
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010214_02

Start Time:	2010-214T00:00:56.471	Stop Time:	2010-214T23:59:57.851
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010215_02

Start Time:	2010-215T00:00:57.850	Stop Time:	2010-215T23:59:25.230
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010216_02

Start Time:	2010-216T00:00:25.230	Stop Time:	2010-216T23:59:48.609
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_2010217_02

Start Time:	2010-217T00:00:48.609	Stop Time:	2010-217T23:59:39.989
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_2010218_02

Start Time:	2010-218T00:00:39.988	Stop Time:	2010-218T23:59:41.368
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010219_02

Start Time:	2010-219T00:00:41.368	Stop Time:	2010-219T23:59:45.748
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010220_02

Start Time:	2010-220T00:00:45.747	Stop Time:	2010-220T23:59:04.127
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010221_02

Start Time:	2010-221T00:00:04.127	Stop Time:	2010-221T23:59:57.506
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010222_02

Start Time:	2010-222T00:01:12.506	Stop Time:	2010-222T23:59:58.886
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010223_02

Start Time:	2010-223T00:01:13.885	Stop Time:	2010-223T23:58:58.266
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010224_02

Start Time:	2010-224T00:01:06.265	Stop Time:	2010-224T23:57:57.645
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010225_02

Start Time:	2010-225T00:00:07.644	Stop Time:	2010-225T23:59:43.024
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010226_02

Start Time:	2010-226T00:01:13.023	Stop Time:	2010-226T23:59:29.403
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010227_02

Start Time:	2010-227T00:00:14.403	Stop Time:	2010-227T23:58:07.783
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010228_02

Start Time:	2010-228T00:00:15.783	Stop Time:	2010-228T23:58:18.163
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010229_02

Start Time:	2010-229T00:00:26.162	Stop Time:	2010-229T23:58:03.542
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010230_02

Start Time:	2010-230T00:00:10.541	Stop Time:	2010-230T16:17:55.120
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_2010231_02

Start Time:	2010-231T01:19:55.886	Stop Time:	2010-231T16:01:56.506
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010232_02

Start Time:	2010-232T01:04:57.272	Stop Time:	2010-232T16:01:57.886
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010233_02

Start Time:	2010-233T01:04:58.652	Stop Time:	2010-233T23:57:54.060
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010234_02

Start Time:	2010-234T00:00:03.059	Stop Time:	2010-234T23:59:36.439
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010235_02

Start Time:	2010-235T00:00:36.438	Stop Time:	2010-235T23:58:44.818
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_2010236_02

Start Time:	2010-236T00:00:51.817	Stop Time:	2010-236T23:59:27.197
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010237_02

Start Time:	2010-237T00:00:27.197	Stop Time:	2010-237T23:58:36.577
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010238_02

Start Time:	2010-238T00:00:44.576	Stop Time:	2010-238T23:59:03.956
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_2010239_02

Start Time:	2010-239T00:00:03.956	Stop Time:	2010-239T23:59:19.336
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010240_02

Start Time:	2010-240T00:01:26.335	Stop Time:	2010-240T23:59:47.715
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010241_02

Start Time:	2010-241T00:00:47.714	Stop Time:	2010-241T23:59:23.094
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010242_02

Start Time:	2010-242T00:01:31.093	Stop Time:	2010-242T23:59:42.474
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010243_02

Start Time:	2010-243T00:00:42.473	Stop Time:	2010-243T23:58:44.853
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010244_02

Start Time:	2010-244T00:00:14.853	Stop Time:	2010-244T23:59:06.233
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_2010245_02

Start Time:	2010-245T00:00:36.232	Stop Time:	2010-245T23:59:07.612
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010246_02

Start Time:	2010-246T00:00:07.612	Stop Time:	2010-246T23:58:53.991
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010247_02

Start Time:	2010-247T00:00:08.991	Stop Time:	2010-247T23:58:54.371
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_2010248_02

Start Time:	2010-248T00:00:09.370	Stop Time:	2010-248T23:58:55.750
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_2010249_02

Start Time:	2010-249T00:00:10.750	Stop Time:	2010-249T23:59:12.130
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010250_02

Start Time:	2010-250T00:00:12.129	Stop Time:	2010-250T23:59:13.509
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010251_02

Start Time:	2010-251T00:00:13.508	Stop Time:	2010-251T23:59:14.888
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_2010252_02

Start Time:	2010-252T00:00:14.888	Stop Time:	2010-252T23:59:16.268
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_2010253_02

Start Time:	2010-253T00:00:16.267	Stop Time:	2010-253T23:59:07.647
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010254_02

Start Time:	2010-254T00:01:15.646	Stop Time:	2010-254T23:59:06.026
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010255_02

Start Time:	2010-255T00:00:06.026	Stop Time:	2010-255T23:58:00.406
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010256_02

Start Time:	2010-256T00:00:08.405	Stop Time:	2010-256T23:59:49.785
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010257_02

Start Time:	2010-257T00:01:19.784	Stop Time:	2010-257T23:59:50.164
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010258_02

Start Time:	2010-258T00:01:20.164	Stop Time:	2010-258T23:59:50.544
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010259_02

Start Time:	2010-259T00:01:20.543	Stop Time:	2010-259T23:59:50.923
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010260_02

Start Time:	2010-260T00:01:20.922	Stop Time:	2010-260T23:59:50.302
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010261_02

Start Time:	2010-261T00:01:20.302	Stop Time:	2010-261T23:59:38.682
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010262_02

Start Time:	2010-262T00:01:08.681	Stop Time:	2010-262T23:58:36.062
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010263_02

Start Time:	2010-263T00:00:06.061	Stop Time:	2010-263T23:59:18.441
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_2010264_02

Start Time:	2010-264T00:00:48.440	Stop Time:	2010-264T23:59:48.820
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010265_02

Start Time:	2010-265T00:00:33.820	Stop Time:	2010-265T23:59:21.200
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010266_02

Start Time:	2010-266T00:00:21.199	Stop Time:	2010-266T23:59:06.579
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010267_02

Start Time:	2010-267T00:00:21.579	Stop Time:	2010-267T23:59:07.958
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010268_02

Start Time:	2010-268T00:00:07.958	Stop Time:	2010-268T23:58:12.338
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010269_02

Start Time:	2010-269T00:00:20.337	Stop Time:	2010-269T23:59:11.717
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010270_02

Start Time:	2010-270T00:01:19.716	Stop Time:	2010-270T23:59:40.096
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010271_02

Start Time:	2010-271T00:00:40.096	Stop Time:	2010-271T23:59:41.476
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010272_02

Start Time:	2010-272T00:00:41.475	Stop Time:	2010-272T23:59:42.855
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010273_02

Start Time:	2010-273T00:00:42.855	Stop Time:	2010-273T23:59:44.235
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010274_02

Start Time:	2010-274T00:00:44.234	Stop Time:	2010-274T18:25:45.758
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010275_02

Start Time:	2010-275T04:46:46.490	Stop Time:	2010-275T23:59:46.993
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010276_02

Start Time:	2010-276T00:00:46.993	Stop Time:	2010-276T23:59:48.373
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010277_02

Start Time:	2010-277T00:00:48.372	Stop Time:	2010-277T23:59:50.752
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010278_02

Start Time:	2010-278T00:00:50.752	Stop Time:	2010-278T23:59:38.132
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_2010279_02

Start Time:	2010-279T00:00:38.131	Stop Time:	2010-279T23:59:29.511
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010280_02

Start Time:	2010-280T00:01:38.510	Stop Time:	2010-280T23:59:54.890
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010281_02

Start Time:	2010-281T00:00:54.890	Stop Time:	2010-281T23:58:21.270
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010282_02

Start Time:	2010-282T00:00:28.269	Stop Time:	2010-282T23:59:43.649
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010283_02

Start Time:	2010-283T00:00:43.649	Stop Time:	2010-283T23:59:21.029
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010284_02

Start Time:	2010-284T00:00:21.028	Stop Time:	2010-284T23:59:25.408
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010285_02

Start Time:	2010-285T00:00:55.407	Stop Time:	2010-285T23:59:29.787
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010286_02

Start Time:	2010-286T00:01:38.786	Stop Time:	2010-286T23:58:32.167
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010287_02

Start Time:	2010-287T00:00:02.166	Stop Time:	2010-287T23:58:49.546
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_2010288_02

Start Time:	2010-288T00:00:19.546	Stop Time:	2010-288T23:59:19.926
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_2010289_02

Start Time:	2010-289T00:01:28.925	Stop Time:	2010-289T23:33:00.316
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010290_02

Start Time:	2010-290T00:40:30.287	Stop Time:	2010-290T23:59:00.684
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_2010291_02

Start Time:	2010-291T00:00:30.684	Stop Time:	2010-291T23:59:01.064
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_2010292_02

Start Time:	2010-292T00:00:31.063	Stop Time:	2010-292T23:59:01.443
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_2010293_02

Start Time:	2010-293T00:00:31.443	Stop Time:	2010-293T23:59:00.823
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010294_02

Start Time:	2010-294T00:00:30.822	Stop Time:	2010-294T23:58:33.202
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_2010295_02

Start Time:	2010-295T00:00:03.202	Stop Time:	2010-295T23:58:33.582
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_2010296_02

Start Time:	2010-296T00:00:03.581	Stop Time:	2010-296T23:58:33.961
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_2010297_02

Start Time:	2010-297T00:00:03.960	Stop Time:	2010-297T23:59:04.340
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010298_02

Start Time:	2010-298T00:00:34.339	Stop Time:	2010-298T23:59:04.720
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010299_02

Start Time:	2010-299T00:00:04.719	Stop Time:	2010-299T23:59:06.099
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010300_02

Start Time:	2010-300T00:00:06.098	Stop Time:	2010-300T23:59:07.478
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010301_02

Start Time:	2010-301T00:00:07.478	Stop Time:	2010-301T23:59:09.858
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_2010302_02

Start Time:	2010-302T00:00:09.857	Stop Time:	2010-302T23:58:40.237
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010303_02

Start Time:	2010-303T00:00:10.237	Stop Time:	2010-303T23:58:40.617
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010304_02

Start Time:	2010-304T00:00:10.616	Stop Time:	2010-304T23:58:40.996
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_2010305_02

Start Time:	2010-305T00:00:10.995	Stop Time:	2010-305T23:58:40.375
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_2010306_02

Start Time:	2010-306T00:00:10.375	Stop Time:	2010-306T21:27:10.820
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010320_02

Start Time:	2010-320T00:00:21.641	Stop Time:	2010-320T23:58:22.095
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_2010321_02

Start Time:	2010-321T00:00:22.094	Stop Time:	2010-321T23:58:23.548
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010322_02

Start Time:	2010-322T00:00:23.547	Stop Time:	2010-322T23:58:25.000
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010323_02

Start Time:	2010-323T00:00:25.000	Stop Time:	2010-323T23:58:26.453
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010324_02

Start Time:	2010-324T00:00:26.452	Stop Time:	2010-324T23:58:27.906
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_2010325_02

Start Time:	2010-325T00:00:27.905	Stop Time:	2010-325T23:58:29.358
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010326_02

Start Time:	2010-326T00:00:29.358	Stop Time:	2010-326T23:58:30.811
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_2010327_02

Start Time:	2010-327T00:00:30.810	Stop Time:	2010-327T23:58:32.264
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010328_02

Start Time:	2010-328T00:00:32.263	Stop Time:	2010-328T23:59:02.716
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010329_02

Start Time:	2010-329T00:00:32.716	Stop Time:	2010-329T23:58:57.169
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010330_02

Start Time:	2010-330T00:01:06.168	Stop Time:	2010-330T23:58:34.622
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010331_02

Start Time:	2010-331T00:00:04.622	Stop Time:	2010-331T23:59:47.074
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010332_02

Start Time:	2010-332T00:01:17.074	Stop Time:	2010-332T23:59:17.527
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010333_02

Start Time:	2010-333T00:00:47.527	Stop Time:	2010-333T23:59:21.980
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_2010334_02

Start Time:	2010-334T00:02:18.979	Stop Time:	2010-334T23:59:30.433
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010335_02

Start Time:	2010-335T00:01:00.432	Stop Time:	2010-335T23:59:58.885
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010336_02

Start Time:	2010-336T00:01:28.885	Stop Time:	2010-336T23:58:49.338
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010337_02

Start Time:	2010-337T00:00:57.338	Stop Time:	2010-337T16:26:09.963
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010340_02

Start Time:	2010-340T00:00:39.696	Stop Time:	2010-340T23:59:10.149
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_2010341_02

Start Time:	2010-341T00:00:40.149	Stop Time:	2010-341T23:59:10.602
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_2010342_02

Start Time:	2010-342T00:00:40.601	Stop Time:	2010-342T23:59:10.055
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010343_02

Start Time:	2010-343T00:00:40.054	Stop Time:	2010-343T23:58:41.529
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010344_02

Start Time:	2010-344T00:00:11.529	Stop Time:	2010-344T23:58:41.984
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010345_02

Start Time:	2010-345T00:00:11.983	Stop Time:	2010-345T23:58:41.438
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010346_02

Start Time:	2010-346T00:00:11.437	Stop Time:	2010-346T23:58:41.892
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010347_02

Start Time:	2010-347T00:00:11.892	Stop Time:	2010-347T23:58:42.346
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_2010348_02

Start Time:	2010-348T00:00:12.346	Stop Time:	2010-348T23:58:42.801
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010349_02

Start Time:	2010-349T00:00:12.800	Stop Time:	2010-349T23:58:42.255
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010350_02

Start Time:	2010-350T00:00:12.254	Stop Time:	2010-350T23:58:42.709
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010351_02

Start Time:	2010-351T00:00:12.709	Stop Time:	2010-351T23:58:43.164
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010352_02

Start Time:	2010-352T00:00:13.163	Stop Time:	2010-352T23:58:42.618
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010353_02

Start Time:	2010-353T00:00:12.617	Stop Time:	2010-353T23:58:43.072
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010354_02

Start Time:	2010-354T00:00:13.072	Stop Time:	2010-354T04:10:12.977
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010355_02

Start Time:	2010-355T00:46:58.508	Stop Time:	2010-355T23:59:43.980
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_2010356_02

Start Time:	2010-356T00:01:13.980	Stop Time:	2010-356T23:59:04.435
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010357_02

Start Time:	2010-357T00:00:34.434	Stop Time:	2010-357T23:59:03.889
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010358_02

Start Time:	2010-358T00:00:33.889	Stop Time:	2010-358T23:59:04.343
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010359_02

Start Time:	2010-359T00:00:34.343	Stop Time:	2010-359T23:59:04.798
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_2010360_02

Start Time:	2010-360T00:00:34.797	Stop Time:	2010-360T23:59:05.252
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_2010361_02

Start Time:	2010-361T00:00:35.251	Stop Time:	2010-361T23:59:04.706
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010362_02

Start Time:	2010-362T00:00:34.706	Stop Time:	2010-362T23:59:05.161
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010363_02

Start Time:	2010-363T00:00:35.160	Stop Time:	2010-363T23:59:05.615
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010364_02

Start Time:	2010-364T00:00:35.614	Stop Time:	2010-364T23:59:05.069
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2010365_02

Start Time:	2010-365T00:00:35.069	Stop Time:	2010-365T23:59:05.523
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value 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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