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Cassini >> MIMI

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

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

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

Citiation Information

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

Top/ DATA/ IANGAVE0_T/ 2005 /

IANGAVE0_T_2005001_02

Start Time:	2005-001T00:00:32.327	Stop Time:	2005-001T23:58:33.765
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_2005002_02

Start Time:	2005-002T00:00:33.765	Stop Time:	2005-002T23:59:35.202
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_2005003_02

Start Time:	2005-003T00:00:35.202	Stop Time:	2005-003T23:59:36.640
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005004_02

Start Time:	2005-004T00:00:36.639	Stop Time:	2005-004T23:59:39.077
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005005_02

Start Time:	2005-005T00:00:39.077	Stop Time:	2005-005T23:59:40.515
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005006_02

Start Time:	2005-006T00:00:40.514	Stop Time:	2005-006T11:41:41.240
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005016_02

Start Time:	2005-016T00:01:29.888	Stop Time:	2005-016T23:58:19.327
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005017_02

Start Time:	2005-017T00:00:19.326	Stop Time:	2005-017T23:59:20.764
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005018_02

Start Time:	2005-018T00:00:20.764	Stop Time:	2005-018T23:59:42.202
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_2005019_02

Start Time:	2005-019T00:00:42.201	Stop Time:	2005-019T23:59:34.639
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005020_02

Start Time:	2005-020T00:00:35.639	Stop Time:	2005-020T23:59:12.077
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005021_02

Start Time:	2005-021T00:00:12.076	Stop Time:	2005-021T23:59:14.514
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_2005022_02

Start Time:	2005-022T00:00:14.514	Stop Time:	2005-022T23:58:26.952
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005023_02

Start Time:	2005-023T00:00:07.951	Stop Time:	2005-023T23:59:22.389
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005024_02

Start Time:	2005-024T00:00:22.388	Stop Time:	2005-024T23:59:21.826
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005025_02

Start Time:	2005-025T00:00:21.826	Stop Time:	2005-025T23:59:23.264
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_2005026_02

Start Time:	2005-026T00:00:23.263	Stop Time:	2005-026T23:59:27.701
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005027_02

Start Time:	2005-027T00:00:27.701	Stop Time:	2005-027T23:59:25.139
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005028_02

Start Time:	2005-028T00:00:25.138	Stop Time:	2005-028T23:59:32.576
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005029_02

Start Time:	2005-029T00:02:31.575	Stop Time:	2005-029T23:58:20.014
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005030_02

Start Time:	2005-030T00:00:01.013	Stop Time:	2005-030T23:58:56.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005031_02

Start Time:	2005-031T00:00:36.451	Stop Time:	2005-031T23:59:02.889
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_2005032_02

Start Time:	2005-032T00:00:03.888	Stop Time:	2005-032T23:59:56.326
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005033_02

Start Time:	2005-033T00:01:36.325	Stop Time:	2005-033T23:45:12.769
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005034_02

Start Time:	2005-034T00:17:42.756	Stop Time:	2005-034T23:59:19.201
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005035_02

Start Time:	2005-035T00:00:19.200	Stop Time:	2005-035T23:59:24.638
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005036_02

Start Time:	2005-036T00:01:06.638	Stop Time:	2005-036T23:59:50.075
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005037_02

Start Time:	2005-037T00:00:50.075	Stop Time:	2005-037T23:59:00.513
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005038_02

Start Time:	2005-038T00:00:40.513	Stop Time:	2005-038T23:59:12.951
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005039_02

Start Time:	2005-039T00:00:12.950	Stop Time:	2005-039T23:59:31.388
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005040_02

Start Time:	2005-040T00:00:31.388	Stop Time:	2005-040T23:59:59.825
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005041_02

Start Time:	2005-041T00:00:59.825	Stop Time:	2005-041T23:59:23.263
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_2005042_02

Start Time:	2005-042T00:01:04.262	Stop Time:	2005-042T23:59:21.700
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005043_02

Start Time:	2005-043T00:00:21.700	Stop Time:	2005-043T23:59:12.138
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005044_02

Start Time:	2005-044T00:00:53.137	Stop Time:	2005-044T23:59:06.575
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_2005045_02

Start Time:	2005-045T00:00:06.575	Stop Time:	2005-045T23:59:57.012
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005046_02

Start Time:	2005-046T00:00:57.012	Stop Time:	2005-046T23:59:59.450
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005047_02

Start Time:	2005-047T00:00:59.449	Stop Time:	2005-047T23:58:59.888
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_2005048_02

Start Time:	2005-048T00:03:00.886	Stop Time:	2005-048T23:59:01.325
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_2005049_02

Start Time:	2005-049T00:00:31.325	Stop Time:	2005-049T23:59:01.763
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005050_02

Start Time:	2005-050T00:00:31.762	Stop Time:	2005-050T23:59:02.200
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_2005051_02

Start Time:	2005-051T00:00:32.199	Stop Time:	2005-051T23:58:58.637
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005052_02

Start Time:	2005-052T00:00:28.637	Stop Time:	2005-052T23:59:49.075
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005053_02

Start Time:	2005-053T00:01:19.074	Stop Time:	2005-053T23:59:48.512
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005054_02

Start Time:	2005-054T00:01:18.511	Stop Time:	2005-054T23:59:22.950
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005055_02

Start Time:	2005-055T00:01:04.949	Stop Time:	2005-055T23:58:21.388
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005056_02

Start Time:	2005-056T00:00:03.387	Stop Time:	2005-056T23:58:43.825
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005057_02

Start Time:	2005-057T00:00:23.824	Stop Time:	2005-057T23:59:36.279
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005058_02

Start Time:	2005-058T00:00:36.285	Stop Time:	2005-058T23:58:58.821
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_2005059_02

Start Time:	2005-059T00:00:39.820	Stop Time:	2005-059T23:59:35.276
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_2005060_02

Start Time:	2005-060T00:01:05.275	Stop Time:	2005-060T23:59:40.731
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_2005061_02

Start Time:	2005-061T00:01:10.731	Stop Time:	2005-061T23:58:19.187
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005062_02

Start Time:	2005-062T00:00:00.186	Stop Time:	2005-062T23:59:51.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005063_02

Start Time:	2005-063T00:01:21.561	Stop Time:	2005-063T22:55:22.031
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005064_02

Start Time:	2005-064T04:21:44.905	Stop Time:	2005-064T23:59:59.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005065_02

Start Time:	2005-065T00:01:39.450	Stop Time:	2005-065T23:59:23.895
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005066_02

Start Time:	2005-066T00:01:04.895	Stop Time:	2005-066T23:59:25.340
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_2005067_02

Start Time:	2005-067T00:00:55.339	Stop Time:	2005-067T23:59:19.784
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005068_02

Start Time:	2005-068T00:00:19.784	Stop Time:	2005-068T23:59:51.229
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005069_02

Start Time:	2005-069T00:01:21.228	Stop Time:	2005-069T23:59:06.673
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005070_02

Start Time:	2005-070T00:00:06.673	Stop Time:	2005-070T23:59:08.118
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005071_02

Start Time:	2005-071T00:00:08.117	Stop Time:	2005-071T23:59:03.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005072_02

Start Time:	2005-072T00:00:33.562	Stop Time:	2005-072T23:59:04.007
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005073_02

Start Time:	2005-073T00:00:34.006	Stop Time:	2005-073T23:59:04.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005074_02

Start Time:	2005-074T00:00:34.451	Stop Time:	2005-074T23:58:30.896
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005075_02

Start Time:	2005-075T00:01:29.895	Stop Time:	2005-075T23:58:45.340
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_2005076_02

Start Time:	2005-076T00:00:26.339	Stop Time:	2005-076T23:59:58.784
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005077_02

Start Time:	2005-077T00:01:38.783	Stop Time:	2005-077T23:59:36.229
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005078_02

Start Time:	2005-078T00:01:16.228	Stop Time:	2005-078T23:59:32.673
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005079_02

Start Time:	2005-079T00:00:32.673	Stop Time:	2005-079T23:59:34.118
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005080_02

Start Time:	2005-080T00:00:34.117	Stop Time:	2005-080T23:58:43.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005081_02

Start Time:	2005-081T00:00:24.562	Stop Time:	2005-081T23:59:42.006
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005082_02

Start Time:	2005-082T00:01:23.006	Stop Time:	2005-082T23:59:10.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005083_02

Start Time:	2005-083T00:00:51.450	Stop Time:	2005-083T23:58:30.896
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005084_02

Start Time:	2005-084T00:00:12.895	Stop Time:	2005-084T23:59:02.340
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_2005085_02

Start Time:	2005-085T00:00:43.339	Stop Time:	2005-085T23:58:48.785
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_2005086_02

Start Time:	2005-086T00:00:29.784	Stop Time:	2005-086T23:58:50.229
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005087_02

Start Time:	2005-087T00:00:31.228	Stop Time:	2005-087T23:58:48.673
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005088_02

Start Time:	2005-088T00:00:18.673	Stop Time:	2005-088T23:59:19.118
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005089_02

Start Time:	2005-089T00:00:19.117	Stop Time:	2005-089T23:58:50.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005090_02

Start Time:	2005-090T00:00:20.562	Stop Time:	2005-090T23:59:21.007
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005091_02

Start Time:	2005-091T00:00:21.006	Stop Time:	2005-091T23:59:22.451
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005092_02

Start Time:	2005-092T00:00:22.451	Stop Time:	2005-092T23:59:09.896
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005093_02

Start Time:	2005-093T00:00:50.895	Stop Time:	2005-093T23:59:52.340
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_2005094_02

Start Time:	2005-094T00:00:52.339	Stop Time:	2005-094T23:59:13.784
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005095_02

Start Time:	2005-095T00:00:13.784	Stop Time:	2005-095T23:58:38.229
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005096_02

Start Time:	2005-096T00:00:19.228	Stop Time:	2005-096T23:59:19.673
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005097_02

Start Time:	2005-097T00:01:00.673	Stop Time:	2005-097T23:59:06.118
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005098_02

Start Time:	2005-098T00:00:46.117	Stop Time:	2005-098T23:59:02.562
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005099_02

Start Time:	2005-099T00:00:02.562	Stop Time:	2005-099T23:59:04.007
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005100_02

Start Time:	2005-100T00:00:04.006	Stop Time:	2005-100T23:58:32.518
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005101_02

Start Time:	2005-101T00:00:13.517	Stop Time:	2005-101T23:59:51.964
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005102_02

Start Time:	2005-102T00:01:31.963	Stop Time:	2005-102T23:59:27.410
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005103_02

Start Time:	2005-103T00:01:38.409	Stop Time:	2005-103T23:58:20.857
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_2005104_02

Start Time:	2005-104T00:00:01.856	Stop Time:	2005-104T23:59:16.303
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005105_02

Start Time:	2005-105T00:00:46.302	Stop Time:	2005-105T23:59:11.749
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005106_02

Start Time:	2005-106T00:00:11.749	Stop Time:	2005-106T23:59:19.195
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_2005107_02

Start Time:	2005-107T00:00:19.195	Stop Time:	2005-107T23:59:58.641
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005108_02

Start Time:	2005-108T00:01:28.641	Stop Time:	2005-108T23:58:50.088
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005109_02

Start Time:	2005-109T00:00:29.087	Stop Time:	2005-109T23:59:10.534
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005110_02

Start Time:	2005-110T00:00:40.533	Stop Time:	2005-110T23:59:44.980
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_2005111_02

Start Time:	2005-111T00:01:14.979	Stop Time:	2005-111T23:59:55.426
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005112_02

Start Time:	2005-112T00:00:55.426	Stop Time:	2005-112T23:59:00.873
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005113_02

Start Time:	2005-113T00:00:00.872	Stop Time:	2005-113T23:59:02.319
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005114_02

Start Time:	2005-114T00:00:32.319	Stop Time:	2005-114T23:59:20.765
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_2005115_02

Start Time:	2005-115T00:01:02.765	Stop Time:	2005-115T23:59:28.212
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005116_02

Start Time:	2005-116T00:01:39.211	Stop Time:	2005-116T23:59:24.658
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005117_02

Start Time:	2005-117T00:01:05.657	Stop Time:	2005-117T23:59:04.104
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005118_02

Start Time:	2005-118T00:00:45.104	Stop Time:	2005-118T23:59:42.550
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005119_02

Start Time:	2005-119T00:01:30.550	Stop Time:	2005-119T23:58:52.997
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005120_02

Start Time:	2005-120T00:00:22.996	Stop Time:	2005-120T23:58:53.443
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_2005121_02

Start Time:	2005-121T00:00:23.442	Stop Time:	2005-121T23:59:27.889
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_2005122_02

Start Time:	2005-122T00:00:57.889	Stop Time:	2005-122T23:59:17.335
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005123_02

Start Time:	2005-123T00:00:47.335	Stop Time:	2005-123T23:59:18.782
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005124_02

Start Time:	2005-124T00:00:18.781	Stop Time:	2005-124T23:59:11.228
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_2005125_02

Start Time:	2005-125T00:00:11.228	Stop Time:	2005-125T23:58:52.674
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005126_02

Start Time:	2005-126T00:00:33.674	Stop Time:	2005-126T23:59:56.120
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_2005127_02

Start Time:	2005-127T00:01:26.120	Stop Time:	2005-127T23:58:17.567
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005128_02

Start Time:	2005-128T00:00:18.566	Stop Time:	2005-128T23:59:53.013
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005129_02

Start Time:	2005-129T00:01:34.012	Stop Time:	2005-129T23:58:37.460
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005130_02

Start Time:	2005-130T00:00:17.459	Stop Time:	2005-130T23:59:59.905
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005131_02

Start Time:	2005-131T00:01:29.905	Stop Time:	2005-131T23:58:30.352
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005132_02

Start Time:	2005-132T00:00:00.352	Stop Time:	2005-132T23:58:30.798
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_2005133_02

Start Time:	2005-133T00:00:00.798	Stop Time:	2005-133T23:58:31.245
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_2005134_02

Start Time:	2005-134T00:00:01.244	Stop Time:	2005-134T23:59:32.691
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_2005135_02

Start Time:	2005-135T00:01:12.690	Stop Time:	2005-135T23:59:52.137
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_2005136_02

Start Time:	2005-136T00:00:52.136	Stop Time:	2005-136T23:58:47.583
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_2005137_02

Start Time:	2005-137T00:00:28.583	Stop Time:	2005-137T23:59:15.029
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_2005138_02

Start Time:	2005-138T00:00:15.029	Stop Time:	2005-138T23:59:35.476
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_2005139_02

Start Time:	2005-139T00:02:34.474	Stop Time:	2005-139T23:58:34.922
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_2005140_02

Start Time:	2005-140T00:00:04.922	Stop Time:	2005-140T23:58:35.369
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005141_02

Start Time:	2005-141T00:00:05.368	Stop Time:	2005-141T23:59:05.815
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005142_02

Start Time:	2005-142T00:00:35.814	Stop Time:	2005-142T23:59:06.261
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005143_02

Start Time:	2005-143T00:00:36.260	Stop Time:	2005-143T23:59:14.707
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005144_02

Start Time:	2005-144T00:00:55.706	Stop Time:	2005-144T23:58:44.154
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005145_02

Start Time:	2005-145T00:00:14.153	Stop Time:	2005-145T23:59:00.600
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005146_02

Start Time:	2005-146T00:00:00.599	Stop Time:	2005-146T23:59:02.046
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005147_02

Start Time:	2005-147T00:00:02.046	Stop Time:	2005-147T23:59:06.492
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_2005148_02

Start Time:	2005-148T00:00:06.492	Stop Time:	2005-148T23:59:36.938
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_2005149_02

Start Time:	2005-149T00:01:06.938	Stop Time:	2005-149T23:59:31.385
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005150_02

Start Time:	2005-150T00:01:12.384	Stop Time:	2005-150T23:59:05.831
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005151_02

Start Time:	2005-151T00:00:45.830	Stop Time:	2005-151T23:58:22.337
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005152_02

Start Time:	2005-152T00:00:03.337	Stop Time:	2005-152T23:58:33.786
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005153_02

Start Time:	2005-153T00:00:13.786	Stop Time:	2005-153T23:59:42.235
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_2005154_02

Start Time:	2005-154T00:01:23.235	Stop Time:	2005-154T23:59:04.685
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005155_02

Start Time:	2005-155T00:00:45.684	Stop Time:	2005-155T23:58:56.134
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005156_02

Start Time:	2005-156T00:00:26.134	Stop Time:	2005-156T23:58:56.584
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005157_02

Start Time:	2005-157T00:00:26.583	Stop Time:	2005-157T23:58:37.033
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_2005158_02

Start Time:	2005-158T00:00:18.032	Stop Time:	2005-158T23:58:45.482
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005159_02

Start Time:	2005-159T00:00:15.482	Stop Time:	2005-159T23:59:15.931
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005160_02

Start Time:	2005-160T00:00:45.931	Stop Time:	2005-160T23:59:10.381
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005161_02

Start Time:	2005-161T00:00:40.380	Stop Time:	2005-161T23:58:56.830
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005162_02

Start Time:	2005-162T00:00:26.829	Stop Time:	2005-162T23:59:50.279
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005163_02

Start Time:	2005-163T00:00:50.279	Stop Time:	2005-163T23:59:34.728
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_2005164_02

Start Time:	2005-164T00:01:15.728	Stop Time:	2005-164T23:59:04.178
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005165_02

Start Time:	2005-165T00:00:34.177	Stop Time:	2005-165T23:59:53.627
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_2005166_02

Start Time:	2005-166T00:01:35.626	Stop Time:	2005-166T23:58:47.077
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005167_02

Start Time:	2005-167T00:00:17.076	Stop Time:	2005-167T23:59:35.526
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005168_02

Start Time:	2005-168T00:01:15.525	Stop Time:	2005-168T23:58:35.975
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005169_02

Start Time:	2005-169T00:00:05.975	Stop Time:	2005-169T23:59:59.424
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005170_02

Start Time:	2005-170T00:01:29.423	Stop Time:	2005-170T23:59:55.873
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005171_02

Start Time:	2005-171T00:01:25.873	Stop Time:	2005-171T23:58:27.323
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005172_02

Start Time:	2005-172T00:00:08.322	Stop Time:	2005-172T23:59:40.772
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005173_02

Start Time:	2005-173T00:01:10.771	Stop Time:	2005-173T23:58:40.222
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005174_02

Start Time:	2005-174T00:00:21.221	Stop Time:	2005-174T23:59:40.671
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005175_02

Start Time:	2005-175T00:01:10.670	Stop Time:	2005-175T23:59:25.120
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_2005176_02

Start Time:	2005-176T00:00:25.120	Stop Time:	2005-176T23:59:20.569
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005177_02

Start Time:	2005-177T00:01:01.569	Stop Time:	2005-177T23:59:53.018
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005178_02

Start Time:	2005-178T00:01:23.018	Stop Time:	2005-178T23:59:52.468
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005179_02

Start Time:	2005-179T00:01:22.467	Stop Time:	2005-179T23:59:04.917
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005180_02

Start Time:	2005-180T00:00:45.917	Stop Time:	2005-180T23:58:27.367
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005181_02

Start Time:	2005-181T00:00:08.366	Stop Time:	2005-181T23:58:22.816
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_2005182_02

Start Time:	2005-182T00:00:02.815	Stop Time:	2005-182T23:59:03.265
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005183_02

Start Time:	2005-183T00:02:02.264	Stop Time:	2005-183T23:59:39.714
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005184_02

Start Time:	2005-184T00:00:39.714	Stop Time:	2005-184T23:59:25.164
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_2005185_02

Start Time:	2005-185T00:00:25.163	Stop Time:	2005-185T23:58:32.613
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005186_02

Start Time:	2005-186T00:00:02.613	Stop Time:	2005-186T23:57:29.063
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005187_02

Start Time:	2005-187T00:00:28.062	Stop Time:	2005-187T23:58:37.512
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005188_02

Start Time:	2005-188T00:00:17.511	Stop Time:	2005-188T23:59:46.961
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_2005189_02

Start Time:	2005-189T00:01:16.960	Stop Time:	2005-189T23:59:18.410
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005190_02

Start Time:	2005-190T00:00:48.410	Stop Time:	2005-190T23:59:03.859
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_2005191_02

Start Time:	2005-191T00:00:33.859	Stop Time:	2005-191T23:58:40.309
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_2005192_02

Start Time:	2005-192T00:00:10.308	Stop Time:	2005-192T23:59:20.716
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_2005193_02

Start Time:	2005-193T00:00:50.715	Stop Time:	2005-193T23:58:47.163
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_2005194_02

Start Time:	2005-194T00:00:17.162	Stop Time:	2005-194T23:58:28.609
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_2005195_02

Start Time:	2005-195T00:00:09.609	Stop Time:	2005-195T23:58:59.056
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005196_02

Start Time:	2005-196T00:00:29.055	Stop Time:	2005-196T23:59:18.502
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005197_02

Start Time:	2005-197T00:00:48.502	Stop Time:	2005-197T23:59:18.949
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005198_02

Start Time:	2005-198T00:00:48.949	Stop Time:	2005-198T23:58:44.396
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005199_02

Start Time:	2005-199T00:00:14.395	Stop Time:	2005-199T23:59:02.843
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005200_02

Start Time:	2005-200T00:00:32.842	Stop Time:	2005-200T18:25:18.417
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005201_02

Start Time:	2005-201T00:23:27.280	Stop Time:	2005-201T23:59:43.736
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_2005202_02

Start Time:	2005-202T00:01:12.735	Stop Time:	2005-202T23:59:43.182
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005203_02

Start Time:	2005-203T00:01:13.182	Stop Time:	2005-203T23:59:42.629
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_2005204_02

Start Time:	2005-204T00:01:12.628	Stop Time:	2005-204T23:59:43.076
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005205_02

Start Time:	2005-205T00:01:13.075	Stop Time:	2005-205T23:59:43.522
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005206_02

Start Time:	2005-206T00:01:13.522	Stop Time:	2005-206T23:59:43.969
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005207_02

Start Time:	2005-207T00:01:13.968	Stop Time:	2005-207T23:59:29.416
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005208_02

Start Time:	2005-208T00:00:59.415	Stop Time:	2005-208T23:59:43.862
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_2005209_02

Start Time:	2005-209T00:01:13.862	Stop Time:	2005-209T23:59:33.309
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_2005210_02

Start Time:	2005-210T00:01:03.309	Stop Time:	2005-210T23:58:50.756
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005211_02

Start Time:	2005-211T00:00:20.756	Stop Time:	2005-211T23:58:51.203
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005212_02

Start Time:	2005-212T00:00:21.202	Stop Time:	2005-212T23:58:51.650
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005213_02

Start Time:	2005-213T00:00:21.649	Stop Time:	2005-213T23:58:40.096
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_2005214_02

Start Time:	2005-214T00:00:10.096	Stop Time:	2005-214T23:59:08.543
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_2005215_02

Start Time:	2005-215T00:00:38.542	Stop Time:	2005-215T23:59:08.989
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_2005216_02

Start Time:	2005-216T00:00:38.989	Stop Time:	2005-216T23:59:09.436
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_2005217_02

Start Time:	2005-217T00:00:39.436	Stop Time:	2005-217T23:58:52.883
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005218_02

Start Time:	2005-218T00:00:22.882	Stop Time:	2005-218T23:59:20.329
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005219_02

Start Time:	2005-219T00:00:20.329	Stop Time:	2005-219T23:59:55.776
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005220_02

Start Time:	2005-220T00:00:55.775	Stop Time:	2005-220T23:59:53.223
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_2005221_02

Start Time:	2005-221T00:00:53.222	Stop Time:	2005-221T23:58:52.670
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_2005222_02

Start Time:	2005-222T00:00:22.669	Stop Time:	2005-222T23:58:53.116
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005223_02

Start Time:	2005-223T00:00:23.116	Stop Time:	2005-223T23:58:53.563
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005224_02

Start Time:	2005-224T00:00:23.562	Stop Time:	2005-224T23:59:44.009
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005225_02

Start Time:	2005-225T00:01:14.009	Stop Time:	2005-225T23:58:57.456
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005226_02

Start Time:	2005-226T00:00:27.456	Stop Time:	2005-226T23:58:52.903
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_2005227_02

Start Time:	2005-227T00:00:22.902	Stop Time:	2005-227T23:59:20.350
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_2005228_02

Start Time:	2005-228T00:00:50.349	Stop Time:	2005-228T23:59:20.796
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005229_02

Start Time:	2005-229T00:00:20.796	Stop Time:	2005-229T23:59:57.243
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005230_02

Start Time:	2005-230T00:00:57.242	Stop Time:	2005-230T23:59:23.690
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005231_02

Start Time:	2005-231T00:00:23.689	Stop Time:	2005-231T23:59:22.136
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_2005232_02

Start Time:	2005-232T00:00:22.136	Stop Time:	2005-232T23:59:53.583
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_2005233_02

Start Time:	2005-233T00:01:23.582	Stop Time:	2005-233T23:59:08.030
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005234_02

Start Time:	2005-234T00:00:08.029	Stop Time:	2005-234T23:59:09.476
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_2005235_02

Start Time:	2005-235T00:00:09.476	Stop Time:	2005-235T23:58:40.923
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_2005236_02

Start Time:	2005-236T00:00:10.923	Stop Time:	2005-236T23:58:55.370
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005237_02

Start Time:	2005-237T00:00:25.369	Stop Time:	2005-237T23:59:05.816
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_2005238_02

Start Time:	2005-238T00:00:35.816	Stop Time:	2005-238T23:59:06.263
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_2005239_02

Start Time:	2005-239T00:00:36.263	Stop Time:	2005-239T23:59:34.710
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005240_02

Start Time:	2005-240T00:01:04.709	Stop Time:	2005-240T23:58:41.157
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_2005241_02

Start Time:	2005-241T00:00:11.156	Stop Time:	2005-241T23:59:10.603
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005242_02

Start Time:	2005-242T00:00:10.603	Stop Time:	2005-242T23:59:57.050
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005243_02

Start Time:	2005-243T00:00:57.049	Stop Time:	2005-243T23:59:58.496
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005244_02

Start Time:	2005-244T00:01:28.496	Stop Time:	2005-244T17:37:29.090
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_2005245_02

Start Time:	2005-245T03:34:28.861	Stop Time:	2005-245T23:59:09.390
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005246_02

Start Time:	2005-246T00:00:09.390	Stop Time:	2005-246T23:59:26.837
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005247_02

Start Time:	2005-247T00:00:26.836	Stop Time:	2005-247T23:59:18.283
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005248_02

Start Time:	2005-248T00:00:18.283	Stop Time:	2005-248T23:37:19.738
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005249_02

Start Time:	2005-249T11:13:53.471	Stop Time:	2005-249T23:59:02.177
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_2005250_02

Start Time:	2005-250T00:00:32.176	Stop Time:	2005-250T08:08:01.989
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_2005251_02

Start Time:	2005-251T02:50:02.558	Stop Time:	2005-251T23:59:54.070
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_2005252_02

Start Time:	2005-252T00:01:24.069	Stop Time:	2005-252T23:59:41.517
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005253_02

Start Time:	2005-253T00:01:11.516	Stop Time:	2005-253T23:59:40.963
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_2005254_02

Start Time:	2005-254T00:01:10.963	Stop Time:	2005-254T23:59:41.472
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005255_02

Start Time:	2005-255T00:01:11.471	Stop Time:	2005-255T23:59:21.920
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005256_02

Start Time:	2005-256T00:00:51.920	Stop Time:	2005-256T23:59:11.368
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_2005257_02

Start Time:	2005-257T00:00:41.368	Stop Time:	2005-257T23:59:50.816
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_2005258_02

Start Time:	2005-258T00:01:20.815	Stop Time:	2005-258T23:59:47.264
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_2005259_02

Start Time:	2005-259T00:01:17.263	Stop Time:	2005-259T23:59:27.712
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005260_02

Start Time:	2005-260T00:00:57.712	Stop Time:	2005-260T23:58:51.160
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_2005261_02

Start Time:	2005-261T00:00:21.160	Stop Time:	2005-261T23:59:36.608
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005262_02

Start Time:	2005-262T00:01:06.607	Stop Time:	2005-262T17:16:07.211
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_2005263_02

Start Time:	2005-263T03:29:37.975	Stop Time:	2005-263T23:59:37.504
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005264_02

Start Time:	2005-264T00:00:37.504	Stop Time:	2005-264T23:59:14.952
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005265_02

Start Time:	2005-265T00:00:14.952	Stop Time:	2005-265T23:59:57.400
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005266_02

Start Time:	2005-266T00:01:27.399	Stop Time:	2005-266T23:59:24.848
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005267_02

Start Time:	2005-267T00:00:24.848	Stop Time:	2005-267T23:59:34.296
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005268_02

Start Time:	2005-268T00:01:04.295	Stop Time:	2005-268T23:59:34.744
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005269_02

Start Time:	2005-269T00:01:04.743	Stop Time:	2005-269T23:59:13.192
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005270_02

Start Time:	2005-270T00:00:43.191	Stop Time:	2005-270T23:59:12.640
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005271_02

Start Time:	2005-271T00:00:42.639	Stop Time:	2005-271T23:59:13.088
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005272_02

Start Time:	2005-272T00:00:43.087	Stop Time:	2005-272T23:59:05.536
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005273_02

Start Time:	2005-273T00:00:46.535	Stop Time:	2005-273T23:58:50.984
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_2005274_02

Start Time:	2005-274T00:00:20.984	Stop Time:	2005-274T23:58:51.432
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_2005275_02

Start Time:	2005-275T00:00:21.432	Stop Time:	2005-275T23:58:51.880
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_2005276_02

Start Time:	2005-276T00:00:21.880	Stop Time:	2005-276T23:58:50.328
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005277_02

Start Time:	2005-277T00:00:20.328	Stop Time:	2005-277T23:59:07.776
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005278_02

Start Time:	2005-278T00:00:37.775	Stop Time:	2005-278T23:58:54.224
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005279_02

Start Time:	2005-279T00:00:24.224	Stop Time:	2005-279T23:59:20.672
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005280_02

Start Time:	2005-280T00:00:20.672	Stop Time:	2005-280T23:59:05.120
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_2005281_02

Start Time:	2005-281T00:00:05.120	Stop Time:	2005-281T23:59:17.568
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005282_02

Start Time:	2005-282T00:00:07.568	Stop Time:	2005-282T23:59:40.016
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005283_02

Start Time:	2005-283T00:00:40.015	Stop Time:	2005-283T23:58:35.464
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005284_02

Start Time:	2005-284T00:00:05.464	Stop Time:	2005-284T23:59:06.912
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005285_02

Start Time:	2005-285T00:00:06.912	Stop Time:	2005-285T23:59:06.360
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005286_02

Start Time:	2005-286T00:00:36.359	Stop Time:	2005-286T23:59:03.808
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005287_02

Start Time:	2005-287T00:00:03.808	Stop Time:	2005-287T23:59:44.256
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005288_02

Start Time:	2005-288T00:00:44.255	Stop Time:	2005-288T23:59:10.704
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_2005289_02

Start Time:	2005-289T00:00:10.704	Stop Time:	2005-289T23:59:23.152
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005290_02

Start Time:	2005-290T00:00:23.151	Stop Time:	2005-290T23:59:54.600
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005291_02

Start Time:	2005-291T00:00:54.599	Stop Time:	2005-291T23:59:23.048
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005292_02

Start Time:	2005-292T00:02:22.047	Stop Time:	2005-292T23:59:39.496
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005293_02

Start Time:	2005-293T00:00:39.495	Stop Time:	2005-293T23:59:23.944
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005294_02

Start Time:	2005-294T00:01:04.943	Stop Time:	2005-294T23:57:21.393
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005295_02

Start Time:	2005-295T00:15:21.386	Stop Time:	2005-295T23:59:22.840
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_2005296_02

Start Time:	2005-296T00:00:22.839	Stop Time:	2005-296T23:59:24.288
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005297_02

Start Time:	2005-297T00:00:24.287	Stop Time:	2005-297T23:59:25.736
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_2005298_02

Start Time:	2005-298T00:00:25.735	Stop Time:	2005-298T23:57:03.185
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005299_02

Start Time:	2005-299T00:02:53.182	Stop Time:	2005-299T23:59:34.632
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005300_02

Start Time:	2005-300T00:00:34.631	Stop Time:	2005-300T23:59:36.080
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005301_02

Start Time:	2005-301T00:01:06.079	Stop Time:	2005-301T23:59:36.528
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005302_02

Start Time:	2005-302T00:01:06.527	Stop Time:	2005-302T23:59:23.976
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_2005303_02

Start Time:	2005-303T00:00:13.975	Stop Time:	2005-303T23:58:46.424
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005304_02

Start Time:	2005-304T00:00:16.423	Stop Time:	2005-304T23:59:04.872
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005305_02

Start Time:	2005-305T00:00:04.871	Stop Time:	2005-305T23:59:25.320
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005306_02

Start Time:	2005-306T00:00:25.319	Stop Time:	2005-306T23:59:26.768
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005307_02

Start Time:	2005-307T00:00:26.767	Stop Time:	2005-307T23:59:41.216
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005308_02

Start Time:	2005-308T00:01:22.215	Stop Time:	2005-308T23:59:18.664
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005309_02

Start Time:	2005-309T00:00:18.663	Stop Time:	2005-309T23:59:24.112
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005310_02

Start Time:	2005-310T00:01:05.111	Stop Time:	2005-310T23:59:47.559
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005311_02

Start Time:	2005-311T00:01:17.559	Stop Time:	2005-311T23:59:49.007
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005312_02

Start Time:	2005-312T00:00:49.007	Stop Time:	2005-312T23:59:10.456
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005313_02

Start Time:	2005-313T00:00:10.455	Stop Time:	2005-313T23:59:32.904
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005314_02

Start Time:	2005-314T00:00:22.903	Stop Time:	2005-314T23:59:35.352
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005315_02

Start Time:	2005-315T00:00:25.351	Stop Time:	2005-315T23:59:16.800
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005316_02

Start Time:	2005-316T00:00:16.799	Stop Time:	2005-316T23:59:39.247
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005317_02

Start Time:	2005-317T00:00:29.247	Stop Time:	2005-317T23:59:40.695
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005318_02

Start Time:	2005-318T00:00:40.695	Stop Time:	2005-318T23:59:22.144
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005319_02

Start Time:	2005-319T00:00:12.143	Stop Time:	2005-319T23:59:24.592
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005320_02

Start Time:	2005-320T00:00:14.591	Stop Time:	2005-320T23:59:46.039
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_2005321_02

Start Time:	2005-321T00:01:16.039	Stop Time:	2005-321T23:59:51.487
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005322_02

Start Time:	2005-322T00:01:06.487	Stop Time:	2005-322T23:58:47.936
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005323_02

Start Time:	2005-323T00:00:02.935	Stop Time:	2005-323T23:59:10.384
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005324_02

Start Time:	2005-324T00:00:10.383	Stop Time:	2005-324T23:59:01.832
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005325_02

Start Time:	2005-325T00:00:16.831	Stop Time:	2005-325T23:59:23.279
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005326_02

Start Time:	2005-326T00:00:23.279	Stop Time:	2005-326T23:59:49.727
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005327_02

Start Time:	2005-327T00:00:39.727	Stop Time:	2005-327T23:58:51.176
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005328_02

Start Time:	2005-328T00:00:32.175	Stop Time:	2005-328T23:59:41.623
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005329_02

Start Time:	2005-329T00:00:31.623	Stop Time:	2005-329T23:59:08.072
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_2005330_02

Start Time:	2005-330T00:00:38.071	Stop Time:	2005-330T23:59:08.520
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_2005331_02

Start Time:	2005-331T00:00:38.519	Stop Time:	2005-331T23:59:43.967
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005332_02

Start Time:	2005-332T00:01:24.967	Stop Time:	2005-332T23:59:43.415
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005333_02

Start Time:	2005-333T00:00:33.415	Stop Time:	2005-333T23:59:55.863
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005334_02

Start Time:	2005-334T00:01:25.863	Stop Time:	2005-334T23:59:56.311
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005335_02

Start Time:	2005-335T00:01:26.311	Stop Time:	2005-335T23:59:26.759
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005336_02

Start Time:	2005-336T00:00:16.759	Stop Time:	2005-336T23:59:34.207
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005337_02

Start Time:	2005-337T00:01:14.207	Stop Time:	2005-337T23:59:26.655
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_2005338_02

Start Time:	2005-338T00:00:16.655	Stop Time:	2005-338T23:59:00.104
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005339_02

Start Time:	2005-339T00:00:30.103	Stop Time:	2005-339T23:59:03.551
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005340_02

Start Time:	2005-340T00:00:33.551	Stop Time:	2005-340T23:59:56.999
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005341_02

Start Time:	2005-341T00:01:36.998	Stop Time:	2005-341T23:59:59.447
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005342_02

Start Time:	2005-342T00:01:29.447	Stop Time:	2005-342T23:59:32.895
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005343_02

Start Time:	2005-343T00:00:22.895	Stop Time:	2005-343T23:58:51.344
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005344_02

Start Time:	2005-344T00:00:21.343	Stop Time:	2005-344T23:59:40.791
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005345_02

Start Time:	2005-345T00:00:55.791	Stop Time:	2005-345T23:59:02.239
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005346_02

Start Time:	2005-346T00:00:43.239	Stop Time:	2005-346T23:59:56.687
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005347_02

Start Time:	2005-347T00:00:46.687	Stop Time:	2005-347T23:58:57.135
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005348_02

Start Time:	2005-348T00:00:37.135	Stop Time:	2005-348T23:59:33.583
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_2005349_02

Start Time:	2005-349T00:00:23.583	Stop Time:	2005-349T23:59:21.970
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005350_02

Start Time:	2005-350T00:01:01.969	Stop Time:	2005-350T23:59:17.416
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005351_02

Start Time:	2005-351T00:00:07.416	Stop Time:	2005-351T23:59:50.862
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_2005352_02

Start Time:	2005-352T00:01:32.861	Stop Time:	2005-352T23:59:19.308
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005353_02

Start Time:	2005-353T00:00:09.308	Stop Time:	2005-353T23:58:49.754
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_2005354_02

Start Time:	2005-354T00:00:29.753	Stop Time:	2005-354T23:59:30.200
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_2005355_02

Start Time:	2005-355T00:00:30.199	Stop Time:	2005-355T23:59:31.646
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005356_02

Start Time:	2005-356T00:00:31.645	Stop Time:	2005-356T23:58:34.092
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_2005357_02

Start Time:	2005-357T00:00:16.091	Stop Time:	2005-357T23:59:40.538
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005358_02

Start Time:	2005-358T00:00:30.537	Stop Time:	2005-358T23:59:43.984
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_2005359_02

Start Time:	2005-359T00:00:33.983	Stop Time:	2005-359T23:58:47.430
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005360_02

Start Time:	2005-360T00:00:27.429	Stop Time:	2005-360T23:59:40.876
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005361_02

Start Time:	2005-361T00:00:30.875	Stop Time:	2005-361T23:59:05.322
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005362_02

Start Time:	2005-362T00:00:05.321	Stop Time:	2005-362T23:59:10.768
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005363_02

Start Time:	2005-363T00:00:10.767	Stop Time:	2005-363T23:59:34.214
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005364_02

Start Time:	2005-364T00:00:49.213	Stop Time:	2005-364T23:59:34.660
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2005365_02

Start Time:	2005-365T00:01:04.659	Stop Time:	2005-365T23:59:35.106
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value 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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