PDS/PPI Home Page

QUICK SEARCH

Search By Missions

QUICK LINKS

FAQ
Citation Policy
Errata for all volumes
Help for Data Users
Help for Data Reviewers
Help for Data Providers

PDS NODES

PDS Home
Atmospheres
Geosciences
Cartography and Imaging Sciences
NAIF - SPICE
Ring-Moon Systems
Small Bodies

Cassini >> MIMI

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

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

CASSINI SATURN MIMI INCA CALIBRATED DATA ARCHIVE

Citiation Information

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

Top/ DATA/ IANGAVE0_T/ 2007 /

IANGAVE0_T_2007001_02

Start Time:	2007-001T00:00:27.176	Stop Time:	2007-001T23:59:13.628
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007002_02

Start Time:	2007-002T00:00:13.628	Stop Time:	2007-002T23:59:44.079
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007003_02

Start Time:	2007-003T00:01:25.078	Stop Time:	2007-003T23:59:58.530
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007004_02

Start Time:	2007-004T00:00:58.530	Stop Time:	2007-004T23:59:46.982
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007005_02

Start Time:	2007-005T00:00:46.981	Stop Time:	2007-005T23:59:48.433
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007006_02

Start Time:	2007-006T00:01:03.432	Stop Time:	2007-006T23:58:19.885
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007007_02

Start Time:	2007-007T00:00:00.884	Stop Time:	2007-007T23:59:05.336
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007008_02

Start Time:	2007-008T00:00:05.335	Stop Time:	2007-008T13:47:41.020
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007009_02

Start Time:	2007-009T04:37:10.681	Stop Time:	2007-009T19:11:11.348
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007010_02

Start Time:	2007-010T04:24:41.137	Stop Time:	2007-010T23:58:36.690
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_2007011_02

Start Time:	2007-011T00:00:06.689	Stop Time:	2007-011T23:59:13.141
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007012_02

Start Time:	2007-012T00:00:43.140	Stop Time:	2007-012T23:59:46.592
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_2007013_02

Start Time:	2007-013T00:01:16.591	Stop Time:	2007-013T23:59:48.043
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007014_02

Start Time:	2007-014T00:01:18.042	Stop Time:	2007-014T23:59:48.494
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007015_02

Start Time:	2007-015T00:01:03.494	Stop Time:	2007-015T23:59:22.946
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007016_02

Start Time:	2007-016T00:00:22.945	Stop Time:	2007-016T23:59:24.397
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007017_02

Start Time:	2007-017T00:00:24.397	Stop Time:	2007-017T23:59:38.848
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_2007018_02

Start Time:	2007-018T00:00:23.848	Stop Time:	2007-018T23:59:30.300
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007019_02

Start Time:	2007-019T00:00:30.299	Stop Time:	2007-019T23:59:04.751
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007020_02

Start Time:	2007-020T00:00:04.751	Stop Time:	2007-020T23:59:56.202
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_2007021_02

Start Time:	2007-021T00:00:56.202	Stop Time:	2007-021T23:59:57.653
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007022_02

Start Time:	2007-022T00:00:57.653	Stop Time:	2007-022T23:59:14.105
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007023_02

Start Time:	2007-023T00:00:14.104	Stop Time:	2007-023T23:58:26.556
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007024_02

Start Time:	2007-024T00:00:07.556	Stop Time:	2007-024T23:58:35.008
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007025_02

Start Time:	2007-025T00:00:05.007	Stop Time:	2007-025T22:50:18.503
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007026_02

Start Time:	2007-026T03:39:48.393	Stop Time:	2007-026T23:58:47.930
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007027_02

Start Time:	2007-027T00:00:17.930	Stop Time:	2007-027T23:58:52.384
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_2007028_02

Start Time:	2007-028T00:00:22.383	Stop Time:	2007-028T23:59:09.837
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_2007029_02

Start Time:	2007-029T00:00:39.836	Stop Time:	2007-029T23:59:55.290
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007030_02

Start Time:	2007-030T00:01:25.289	Stop Time:	2007-030T23:59:26.743
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007031_02

Start Time:	2007-031T00:00:26.743	Stop Time:	2007-031T23:59:14.196
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007032_02

Start Time:	2007-032T00:00:14.196	Stop Time:	2007-032T23:59:45.650
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_2007033_02

Start Time:	2007-033T00:00:45.649	Stop Time:	2007-033T23:59:07.103
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007034_02

Start Time:	2007-034T00:00:48.102	Stop Time:	2007-034T23:59:43.556
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007035_02

Start Time:	2007-035T00:00:28.556	Stop Time:	2007-035T23:59:30.009
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_2007036_02

Start Time:	2007-036T00:00:45.009	Stop Time:	2007-036T23:59:30.463
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007037_02

Start Time:	2007-037T00:00:30.462	Stop Time:	2007-037T23:59:16.916
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007038_02

Start Time:	2007-038T00:00:16.916	Stop Time:	2007-038T23:59:18.369
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_2007039_02

Start Time:	2007-039T00:00:18.369	Stop Time:	2007-039T23:54:17.824
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007040_02

Start Time:	2007-040T00:36:19.808	Stop Time:	2007-040T23:59:59.275
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007041_02

Start Time:	2007-041T00:00:59.275	Stop Time:	2007-041T23:59:31.729
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007042_02

Start Time:	2007-042T00:00:16.729	Stop Time:	2007-042T23:59:35.182
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_2007043_02

Start Time:	2007-043T00:00:20.182	Stop Time:	2007-043T23:58:35.636
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007044_02

Start Time:	2007-044T00:00:16.635	Stop Time:	2007-044T21:40:55.141
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007045_02

Start Time:	2007-045T00:44:20.072	Stop Time:	2007-045T14:43:34.753
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007046_02

Start Time:	2007-046T00:21:04.534	Stop Time:	2007-046T23:58:14.996
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007047_02

Start Time:	2007-047T00:01:13.995	Stop Time:	2007-047T23:59:20.449
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007048_02

Start Time:	2007-048T00:00:05.448	Stop Time:	2007-048T23:59:05.902
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007049_02

Start Time:	2007-049T00:00:05.901	Stop Time:	2007-049T23:59:40.355
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007050_02

Start Time:	2007-050T00:00:40.355	Stop Time:	2007-050T23:59:11.808
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_2007051_02

Start Time:	2007-051T00:00:11.808	Stop Time:	2007-051T19:10:42.371
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007052_02

Start Time:	2007-052T00:10:42.257	Stop Time:	2007-052T10:37:58.019
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007053_02

Start Time:	2007-053T02:48:59.650	Stop Time:	2007-053T12:47:29.423
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007054_02

Start Time:	2007-054T01:11:30.141	Stop Time:	2007-054T23:59:32.621
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007055_02

Start Time:	2007-055T00:00:32.621	Stop Time:	2007-055T23:59:13.075
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_2007056_02

Start Time:	2007-056T00:00:13.074	Stop Time:	2007-056T23:59:14.528
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_2007057_02

Start Time:	2007-057T00:00:14.527	Stop Time:	2007-057T23:59:15.981
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007058_02

Start Time:	2007-058T00:00:15.981	Stop Time:	2007-058T23:59:09.434
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007059_02

Start Time:	2007-059T00:00:09.434	Stop Time:	2007-059T23:59:00.888
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_2007060_02

Start Time:	2007-060T00:00:00.887	Stop Time:	2007-060T23:59:38.341
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007061_02

Start Time:	2007-061T00:00:38.340	Stop Time:	2007-061T11:13:46.085
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007062_02

Start Time:	2007-062T00:27:15.783	Stop Time:	2007-062T10:12:26.561
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007063_02

Start Time:	2007-063T00:37:56.233	Stop Time:	2007-063T23:59:27.701
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_2007064_02

Start Time:	2007-064T00:01:07.700	Stop Time:	2007-064T23:59:04.154
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_2007065_02

Start Time:	2007-065T00:00:46.153	Stop Time:	2007-065T23:59:19.607
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007066_02

Start Time:	2007-066T00:00:34.607	Stop Time:	2007-066T23:59:21.060
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007067_02

Start Time:	2007-067T00:00:21.060	Stop Time:	2007-067T23:59:48.513
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_2007068_02

Start Time:	2007-068T00:00:48.513	Stop Time:	2007-068T23:59:30.967
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_2007069_02

Start Time:	2007-069T00:00:15.967	Stop Time:	2007-069T23:59:02.420
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007070_02

Start Time:	2007-070T00:00:42.420	Stop Time:	2007-070T23:59:44.873
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_2007071_02

Start Time:	2007-071T00:00:29.873	Stop Time:	2007-071T23:59:24.327
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_2007072_02

Start Time:	2007-072T00:00:09.326	Stop Time:	2007-072T23:59:27.780
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007073_02

Start Time:	2007-073T00:00:12.780	Stop Time:	2007-073T23:59:30.233
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007074_02

Start Time:	2007-074T00:00:15.233	Stop Time:	2007-074T23:59:37.686
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007075_02

Start Time:	2007-075T00:00:22.686	Stop Time:	2007-075T23:59:36.140
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007076_02

Start Time:	2007-076T00:01:50.139	Stop Time:	2007-076T23:59:38.593
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007077_02

Start Time:	2007-077T00:00:23.593	Stop Time:	2007-077T23:59:42.046
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_2007078_02

Start Time:	2007-078T00:00:27.046	Stop Time:	2007-078T21:04:57.566
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007079_02

Start Time:	2007-079T00:42:27.483	Stop Time:	2007-079T23:58:52.953
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007080_02

Start Time:	2007-080T00:00:22.952	Stop Time:	2007-080T06:32:43.803
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007081_02

Start Time:	2007-081T13:01:12.109	Stop Time:	2007-081T23:27:00.871
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007082_02

Start Time:	2007-082T01:28:30.825	Stop Time:	2007-082T23:59:01.313
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007083_02

Start Time:	2007-083T00:00:01.312	Stop Time:	2007-083T23:58:40.766
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007084_02

Start Time:	2007-084T00:00:21.765	Stop Time:	2007-084T23:59:41.219
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007085_02

Start Time:	2007-085T00:00:26.219	Stop Time:	2007-085T23:59:44.672
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_2007086_02

Start Time:	2007-086T00:00:29.672	Stop Time:	2007-086T23:59:47.125
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007087_02

Start Time:	2007-087T00:00:32.125	Stop Time:	2007-087T23:59:50.579
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007088_02

Start Time:	2007-088T00:00:35.578	Stop Time:	2007-088T23:59:53.032
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007089_02

Start Time:	2007-089T00:00:38.032	Stop Time:	2007-089T23:58:56.485
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007090_02

Start Time:	2007-090T00:00:38.485	Stop Time:	2007-090T23:59:49.938
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_2007091_02

Start Time:	2007-091T00:00:34.938	Stop Time:	2007-091T23:59:52.392
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007092_02

Start Time:	2007-092T00:00:37.391	Stop Time:	2007-092T23:59:55.845
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007093_02

Start Time:	2007-093T00:00:40.845	Stop Time:	2007-093T23:02:42.320
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_2007096_02

Start Time:	2007-096T00:00:03.205	Stop Time:	2007-096T23:59:19.658
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_2007097_02

Start Time:	2007-097T00:00:04.658	Stop Time:	2007-097T23:59:23.111
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007098_02

Start Time:	2007-098T00:00:08.111	Stop Time:	2007-098T23:59:15.565
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007099_02

Start Time:	2007-099T00:00:30.564	Stop Time:	2007-099T23:59:02.018
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_2007100_02

Start Time:	2007-100T00:00:17.017	Stop Time:	2007-100T23:59:42.449
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007101_02

Start Time:	2007-101T00:01:12.448	Stop Time:	2007-101T23:58:45.902
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007102_02

Start Time:	2007-102T00:00:26.902	Stop Time:	2007-102T23:59:37.355
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007103_02

Start Time:	2007-103T00:00:22.355	Stop Time:	2007-103T23:59:16.808
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_2007104_02

Start Time:	2007-104T00:00:01.808	Stop Time:	2007-104T23:59:20.261
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_2007105_02

Start Time:	2007-105T00:00:05.261	Stop Time:	2007-105T23:59:22.714
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_2007106_02

Start Time:	2007-106T00:00:07.713	Stop Time:	2007-106T23:59:26.167
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007107_02

Start Time:	2007-107T00:01:08.166	Stop Time:	2007-107T23:59:15.620
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007108_02

Start Time:	2007-108T00:00:00.619	Stop Time:	2007-108T23:59:19.072
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_2007109_02

Start Time:	2007-109T00:00:04.072	Stop Time:	2007-109T23:59:21.525
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007110_02

Start Time:	2007-110T00:00:06.525	Stop Time:	2007-110T23:58:58.978
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007111_02

Start Time:	2007-111T00:00:39.978	Stop Time:	2007-111T23:59:04.431
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007112_02

Start Time:	2007-112T00:00:45.431	Stop Time:	2007-112T23:58:38.884
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007113_02

Start Time:	2007-113T00:00:19.884	Stop Time:	2007-113T23:58:59.337
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_2007114_02

Start Time:	2007-114T00:00:40.337	Stop Time:	2007-114T23:59:23.790
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007115_02

Start Time:	2007-115T00:00:23.790	Stop Time:	2007-115T23:58:24.243
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_2007116_02

Start Time:	2007-116T00:00:05.243	Stop Time:	2007-116T23:58:37.696
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007117_02

Start Time:	2007-117T00:00:07.695	Stop Time:	2007-117T23:59:21.149
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007118_02

Start Time:	2007-118T00:00:06.148	Stop Time:	2007-118T23:59:18.602
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007119_02

Start Time:	2007-119T00:00:59.601	Stop Time:	2007-119T23:59:24.054
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007120_02

Start Time:	2007-120T00:00:09.054	Stop Time:	2007-120T23:59:27.507
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007121_02

Start Time:	2007-121T00:00:12.507	Stop Time:	2007-121T23:23:29.974
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007122_02

Start Time:	2007-122T12:09:16.683	Stop Time:	2007-122T23:59:47.413
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007123_02

Start Time:	2007-123T00:00:32.413	Stop Time:	2007-123T23:58:44.866
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007124_02

Start Time:	2007-124T00:00:25.866	Stop Time:	2007-124T23:59:44.319
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_2007125_02

Start Time:	2007-125T00:00:29.319	Stop Time:	2007-125T23:59:47.772
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_2007126_02

Start Time:	2007-126T00:00:32.772	Stop Time:	2007-126T23:59:50.225
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007127_02

Start Time:	2007-127T00:00:35.224	Stop Time:	2007-127T23:58:30.678
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007128_02

Start Time:	2007-128T00:00:12.677	Stop Time:	2007-128T23:59:22.131
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007129_02

Start Time:	2007-129T00:00:22.130	Stop Time:	2007-129T23:59:23.584
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_2007130_02

Start Time:	2007-130T00:00:23.583	Stop Time:	2007-130T23:59:39.036
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007131_02

Start Time:	2007-131T00:00:39.036	Stop Time:	2007-131T23:59:44.489
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007132_02

Start Time:	2007-132T00:01:26.489	Stop Time:	2007-132T23:58:37.943
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007133_02

Start Time:	2007-133T00:00:07.942	Stop Time:	2007-133T23:59:53.395
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007134_02

Start Time:	2007-134T00:00:53.395	Stop Time:	2007-134T23:59:09.848
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_2007135_02

Start Time:	2007-135T00:00:09.848	Stop Time:	2007-135T23:59:12.301
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007136_02

Start Time:	2007-136T00:00:12.301	Stop Time:	2007-136T23:59:13.754
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_2007137_02

Start Time:	2007-137T00:00:13.754	Stop Time:	2007-137T23:59:30.207
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_2007138_02

Start Time:	2007-138T00:00:30.206	Stop Time:	2007-138T23:59:19.660
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_2007139_02

Start Time:	2007-139T00:00:34.659	Stop Time:	2007-139T23:59:23.113
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007140_02

Start Time:	2007-140T00:00:38.112	Stop Time:	2007-140T23:59:50.565
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007141_02

Start Time:	2007-141T00:00:50.565	Stop Time:	2007-141T23:59:53.018
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_2007142_02

Start Time:	2007-142T00:00:53.018	Stop Time:	2007-142T23:59:22.471
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007143_02

Start Time:	2007-143T00:00:37.471	Stop Time:	2007-143T23:59:31.924
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007144_02

Start Time:	2007-144T00:00:31.924	Stop Time:	2007-144T23:59:48.377
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007145_02

Start Time:	2007-145T00:00:48.377	Stop Time:	2007-145T23:59:04.830
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_2007146_02

Start Time:	2007-146T00:00:04.830	Stop Time:	2007-146T23:59:50.283
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_2007147_02

Start Time:	2007-147T00:01:05.282	Stop Time:	2007-147T23:59:34.736
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_2007148_02

Start Time:	2007-148T00:01:15.735	Stop Time:	2007-148T23:59:36.189
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007149_02

Start Time:	2007-149T00:01:06.188	Stop Time:	2007-149T23:59:06.642
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007150_02

Start Time:	2007-150T00:00:06.642	Stop Time:	2007-150T23:59:00.095
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007151_02

Start Time:	2007-151T00:00:42.094	Stop Time:	2007-151T23:57:02.549
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007152_02

Start Time:	2007-152T00:00:01.547	Stop Time:	2007-152T23:59:29.001
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007153_02

Start Time:	2007-153T00:00:29.000	Stop Time:	2007-153T23:59:40.453
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007154_02

Start Time:	2007-154T00:00:40.453	Stop Time:	2007-154T23:58:22.907
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007155_02

Start Time:	2007-155T00:00:03.906	Stop Time:	2007-155T23:59:05.359
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007156_02

Start Time:	2007-156T00:00:46.359	Stop Time:	2007-156T23:59:26.812
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007157_02

Start Time:	2007-157T00:00:26.812	Stop Time:	2007-157T23:59:28.265
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_2007158_02

Start Time:	2007-158T00:00:28.265	Stop Time:	2007-158T23:58:55.718
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007159_02

Start Time:	2007-159T00:00:35.718	Stop Time:	2007-159T21:03:36.238
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007160_02

Start Time:	2007-160T03:09:49.099	Stop Time:	2007-160T23:59:49.624
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007161_02

Start Time:	2007-161T00:00:49.623	Stop Time:	2007-161T23:59:36.077
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_2007162_02

Start Time:	2007-162T00:00:51.076	Stop Time:	2007-162T23:59:07.530
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007163_02

Start Time:	2007-163T00:00:07.529	Stop Time:	2007-163T23:59:57.982
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007164_02

Start Time:	2007-164T00:00:42.982	Stop Time:	2007-164T23:59:29.436
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_2007165_02

Start Time:	2007-165T00:00:29.435	Stop Time:	2007-165T23:59:22.888
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_2007166_02

Start Time:	2007-166T00:00:07.888	Stop Time:	2007-166T23:59:25.341
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007167_02

Start Time:	2007-167T00:00:10.341	Stop Time:	2007-167T23:59:27.794
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007168_02

Start Time:	2007-168T00:00:12.794	Stop Time:	2007-168T23:59:22.247
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_2007169_02

Start Time:	2007-169T00:00:07.247	Stop Time:	2007-169T23:59:26.700
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_2007170_02

Start Time:	2007-170T00:00:11.700	Stop Time:	2007-170T23:59:29.153
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007171_02

Start Time:	2007-171T00:00:14.153	Stop Time:	2007-171T23:59:35.606
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007172_02

Start Time:	2007-172T00:01:16.605	Stop Time:	2007-172T23:59:52.059
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007173_02

Start Time:	2007-173T00:00:37.058	Stop Time:	2007-173T23:59:54.512
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_2007174_02

Start Time:	2007-174T00:00:39.511	Stop Time:	2007-174T23:59:00.965
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007175_02

Start Time:	2007-175T00:00:40.964	Stop Time:	2007-175T23:59:27.418
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007176_02

Start Time:	2007-176T00:00:12.417	Stop Time:	2007-176T23:59:20.871
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007177_02

Start Time:	2007-177T00:01:02.870	Stop Time:	2007-177T23:59:05.324
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007178_02

Start Time:	2007-178T00:00:20.323	Stop Time:	2007-178T23:59:25.776
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_2007179_02

Start Time:	2007-179T00:00:25.776	Stop Time:	2007-179T23:59:45.229
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_2007180_02

Start Time:	2007-180T00:01:15.229	Stop Time:	2007-180T23:59:15.682
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007181_02

Start Time:	2007-181T00:00:15.682	Stop Time:	2007-181T23:59:46.135
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_2007182_02

Start Time:	2007-182T00:00:31.135	Stop Time:	2007-182T23:59:27.588
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007183_02

Start Time:	2007-183T00:01:07.587	Stop Time:	2007-183T23:58:55.041
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007184_02

Start Time:	2007-184T00:00:35.040	Stop Time:	2007-184T23:59:52.494
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007185_02

Start Time:	2007-185T00:00:52.493	Stop Time:	2007-185T23:59:48.947
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007186_02

Start Time:	2007-186T00:00:48.946	Stop Time:	2007-186T23:59:31.400
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_2007187_02

Start Time:	2007-187T00:01:11.399	Stop Time:	2007-187T23:59:19.853
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007188_02

Start Time:	2007-188T00:00:59.852	Stop Time:	2007-188T23:58:26.306
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007189_02

Start Time:	2007-189T00:00:07.305	Stop Time:	2007-189T23:59:42.758
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007190_02

Start Time:	2007-190T00:00:27.758	Stop Time:	2007-190T23:59:46.211
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_2007191_02

Start Time:	2007-191T00:00:31.211	Stop Time:	2007-191T23:58:46.664
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_2007192_02

Start Time:	2007-192T00:00:27.664	Stop Time:	2007-192T23:59:33.117
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007193_02

Start Time:	2007-193T00:01:14.116	Stop Time:	2007-193T23:59:13.570
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007194_02

Start Time:	2007-194T00:00:53.569	Stop Time:	2007-194T23:59:49.023
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007195_02

Start Time:	2007-195T00:00:34.022	Stop Time:	2007-195T23:59:58.476
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_2007196_02

Start Time:	2007-196T00:00:43.475	Stop Time:	2007-196T23:59:16.929
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007197_02

Start Time:	2007-197T00:00:01.928	Stop Time:	2007-197T23:59:19.382
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007198_02

Start Time:	2007-198T00:00:04.381	Stop Time:	2007-198T23:59:25.835
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007199_02

Start Time:	2007-199T00:01:06.834	Stop Time:	2007-199T23:59:20.287
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007200_02

Start Time:	2007-200T00:00:05.287	Stop Time:	2007-200T23:59:22.740
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007201_02

Start Time:	2007-201T00:00:07.740	Stop Time:	2007-201T09:42:15.519
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007202_02

Start Time:	2007-202T02:15:16.142	Stop Time:	2007-202T23:59:02.646
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_2007203_02

Start Time:	2007-203T00:00:17.646	Stop Time:	2007-203T23:58:58.099
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007204_02

Start Time:	2007-204T00:00:39.099	Stop Time:	2007-204T23:59:18.552
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007205_02

Start Time:	2007-205T00:00:33.552	Stop Time:	2007-205T23:59:50.005
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007206_02

Start Time:	2007-206T00:01:05.004	Stop Time:	2007-206T23:59:32.458
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007207_02

Start Time:	2007-207T00:00:32.457	Stop Time:	2007-207T23:58:32.911
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007208_02

Start Time:	2007-208T00:00:13.910	Stop Time:	2007-208T23:57:34.364
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007209_02

Start Time:	2007-209T00:00:33.363	Stop Time:	2007-209T23:59:56.816
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_2007210_02

Start Time:	2007-210T00:00:56.816	Stop Time:	2007-210T23:59:58.269
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007211_02

Start Time:	2007-211T00:00:58.269	Stop Time:	2007-211T23:57:14.723
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007212_02

Start Time:	2007-212T00:00:13.722	Stop Time:	2007-212T23:59:31.175
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007213_02

Start Time:	2007-213T00:00:31.175	Stop Time:	2007-213T23:59:46.628
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007214_02

Start Time:	2007-214T00:00:46.628	Stop Time:	2007-214T23:59:35.081
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007215_02

Start Time:	2007-215T00:00:35.081	Stop Time:	2007-215T23:57:31.535
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007216_02

Start Time:	2007-216T00:00:30.534	Stop Time:	2007-216T23:59:46.987
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007217_02

Start Time:	2007-217T00:00:46.986	Stop Time:	2007-217T23:59:49.440
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007218_02

Start Time:	2007-218T00:00:49.439	Stop Time:	2007-218T23:59:30.893
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007219_02

Start Time:	2007-219T00:00:30.892	Stop Time:	2007-219T23:59:21.346
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007220_02

Start Time:	2007-220T00:00:21.345	Stop Time:	2007-220T23:59:18.799
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007221_02

Start Time:	2007-221T00:00:18.798	Stop Time:	2007-221T23:59:34.251
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007222_02

Start Time:	2007-222T00:00:34.251	Stop Time:	2007-222T23:59:35.704
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_2007223_02

Start Time:	2007-223T00:00:35.704	Stop Time:	2007-223T23:59:37.157
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_2007224_02

Start Time:	2007-224T00:01:07.157	Stop Time:	2007-224T23:59:54.610
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007225_02

Start Time:	2007-225T00:01:24.610	Stop Time:	2007-225T23:59:55.063
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_2007226_02

Start Time:	2007-226T00:01:25.062	Stop Time:	2007-226T23:59:27.516
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007227_02

Start Time:	2007-227T00:00:57.516	Stop Time:	2007-227T23:59:34.969
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_2007228_02

Start Time:	2007-228T00:01:04.968	Stop Time:	2007-228T23:59:39.422
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007229_02

Start Time:	2007-229T00:01:09.421	Stop Time:	2007-229T23:59:33.875
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007230_02

Start Time:	2007-230T00:01:03.874	Stop Time:	2007-230T23:59:46.328
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_2007231_02

Start Time:	2007-231T00:01:27.327	Stop Time:	2007-231T23:59:02.781
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007232_02

Start Time:	2007-232T00:00:02.780	Stop Time:	2007-232T23:59:04.234
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007233_02

Start Time:	2007-233T00:00:04.233	Stop Time:	2007-233T23:59:05.687
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_2007234_02

Start Time:	2007-234T00:00:05.686	Stop Time:	2007-234T23:59:07.140
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007235_02

Start Time:	2007-235T00:00:07.139	Stop Time:	2007-235T23:59:08.592
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_2007236_02

Start Time:	2007-236T00:00:08.592	Stop Time:	2007-236T23:59:56.045
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007237_02

Start Time:	2007-237T00:01:38.044	Stop Time:	2007-237T23:59:02.498
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007238_02

Start Time:	2007-238T00:00:32.498	Stop Time:	2007-238T23:59:20.951
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_2007239_02

Start Time:	2007-239T00:00:50.951	Stop Time:	2007-239T23:59:21.404
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007240_02

Start Time:	2007-240T00:00:21.404	Stop Time:	2007-240T23:59:22.857
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_2007241_02

Start Time:	2007-241T00:00:22.857	Stop Time:	2007-241T23:59:09.310
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007242_02

Start Time:	2007-242T00:00:09.310	Stop Time:	2007-242T23:59:44.763
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_2007243_02

Start Time:	2007-243T00:01:14.762	Stop Time:	2007-243T23:59:46.215
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007244_02

Start Time:	2007-244T00:00:46.215	Stop Time:	2007-244T23:59:31.668
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007245_02

Start Time:	2007-245T00:01:01.668	Stop Time:	2007-245T23:58:57.122
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007246_02

Start Time:	2007-246T00:00:27.121	Stop Time:	2007-246T23:58:30.575
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_2007247_02

Start Time:	2007-247T00:00:00.574	Stop Time:	2007-247T23:58:30.028
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007248_02

Start Time:	2007-248T00:00:00.027	Stop Time:	2007-248T23:59:42.480
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007249_02

Start Time:	2007-249T00:01:12.480	Stop Time:	2007-249T23:59:32.933
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007250_02

Start Time:	2007-250T00:01:02.932	Stop Time:	2007-250T23:59:05.386
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007251_02

Start Time:	2007-251T00:00:35.386	Stop Time:	2007-251T23:59:44.839
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007252_02

Start Time:	2007-252T00:01:14.838	Stop Time:	2007-252T23:58:47.292
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007253_02

Start Time:	2007-253T00:00:17.292	Stop Time:	2007-253T23:59:41.745
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007254_02

Start Time:	2007-254T00:01:11.744	Stop Time:	2007-254T05:53:41.610
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007259_02

Start Time:	2007-259T12:20:01.728	Stop Time:	2007-259T23:58:58.462
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007260_02

Start Time:	2007-260T00:00:58.462	Stop Time:	2007-260T23:58:54.915
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007261_02

Start Time:	2007-261T00:00:54.915	Stop Time:	2007-261T23:59:33.368
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_2007262_02

Start Time:	2007-262T00:01:33.367	Stop Time:	2007-262T23:58:29.821
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_2007263_02

Start Time:	2007-263T00:00:29.821	Stop Time:	2007-263T23:58:03.274
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007264_02

Start Time:	2007-264T00:00:03.274	Stop Time:	2007-264T23:59:17.727
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_2007265_02

Start Time:	2007-265T00:01:17.726	Stop Time:	2007-265T23:58:49.180
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007266_02

Start Time:	2007-266T00:00:19.179	Stop Time:	2007-266T23:58:47.633
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007267_02

Start Time:	2007-267T00:00:17.632	Stop Time:	2007-267T23:58:46.086
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007268_02

Start Time:	2007-268T00:00:01.085	Stop Time:	2007-268T23:59:28.538
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_2007269_02

Start Time:	2007-269T00:00:28.538	Stop Time:	2007-269T20:49:29.049
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007270_02

Start Time:	2007-270T14:50:48.638	Stop Time:	2007-270T23:59:26.430
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_2007271_02

Start Time:	2007-271T00:00:26.430	Stop Time:	2007-271T23:59:42.883
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_2007272_02

Start Time:	2007-272T00:00:42.883	Stop Time:	2007-272T23:59:44.336
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007273_02

Start Time:	2007-273T00:00:44.336	Stop Time:	2007-273T21:58:49.836
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007274_02

Start Time:	2007-274T12:53:19.644	Stop Time:	2007-274T13:09:20.490
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007275_02

Start Time:	2007-275T01:13:21.215	Stop Time:	2007-275T07:40:22.068
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007276_02

Start Time:	2007-276T14:17:31.371	Stop Time:	2007-276T23:59:28.150
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007277_02

Start Time:	2007-277T00:00:58.149	Stop Time:	2007-277T23:58:56.603
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_2007278_02

Start Time:	2007-278T00:00:26.603	Stop Time:	2007-278T23:58:50.056
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_2007279_02

Start Time:	2007-279T00:00:20.056	Stop Time:	2007-279T20:04:17.599
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007292_02

Start Time:	2007-292T00:01:16.242	Stop Time:	2007-292T23:59:36.626
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007293_02

Start Time:	2007-293T00:01:06.625	Stop Time:	2007-293T23:59:19.010
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007294_02

Start Time:	2007-294T00:00:49.009	Stop Time:	2007-294T23:58:57.394
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007295_02

Start Time:	2007-295T00:00:27.393	Stop Time:	2007-295T23:59:20.777
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007296_02

Start Time:	2007-296T00:00:20.777	Stop Time:	2007-296T23:59:37.161
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007297_02

Start Time:	2007-297T00:00:37.160	Stop Time:	2007-297T23:59:08.577
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007298_02

Start Time:	2007-298T00:00:08.577	Stop Time:	2007-298T23:59:24.970
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_2007299_02

Start Time:	2007-299T00:00:24.969	Stop Time:	2007-299T23:59:26.362
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007300_02

Start Time:	2007-300T00:00:26.362	Stop Time:	2007-300T23:59:33.754
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_2007301_02

Start Time:	2007-301T00:00:33.754	Stop Time:	2007-301T23:59:27.147
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007302_02

Start Time:	2007-302T00:00:27.146	Stop Time:	2007-302T23:59:27.539
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007303_02

Start Time:	2007-303T00:00:42.539	Stop Time:	2007-303T23:59:57.931
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_2007304_02

Start Time:	2007-304T00:00:57.931	Stop Time:	2007-304T23:59:45.324
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007305_02

Start Time:	2007-305T00:00:30.323	Stop Time:	2007-305T23:59:24.716
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_2007306_02

Start Time:	2007-306T00:00:09.716	Stop Time:	2007-306T23:59:35.109
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007307_02

Start Time:	2007-307T00:00:20.108	Stop Time:	2007-307T23:59:19.501
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007308_02

Start Time:	2007-308T00:00:19.501	Stop Time:	2007-308T23:59:05.893
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007309_02

Start Time:	2007-309T00:00:05.893	Stop Time:	2007-309T23:59:35.286
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007310_02

Start Time:	2007-310T00:00:35.285	Stop Time:	2007-310T23:59:32.631
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007311_02

Start Time:	2007-311T00:00:32.631	Stop Time:	2007-311T23:59:32.021
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007312_02

Start Time:	2007-312T00:00:32.021	Stop Time:	2007-312T23:59:39.411
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007313_02

Start Time:	2007-313T00:00:39.410	Stop Time:	2007-313T23:59:40.800
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_2007314_02

Start Time:	2007-314T00:00:25.800	Stop Time:	2007-314T23:58:45.190
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007315_02

Start Time:	2007-315T00:00:15.189	Stop Time:	2007-315T23:59:09.580
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007316_02

Start Time:	2007-316T00:00:39.579	Stop Time:	2007-316T23:59:19.969
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_2007317_02

Start Time:	2007-317T00:00:49.968	Stop Time:	2007-317T23:59:57.358
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007318_02

Start Time:	2007-318T00:01:27.358	Stop Time:	2007-318T23:58:56.748
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007319_02

Start Time:	2007-319T00:00:26.748	Stop Time:	2007-319T23:59:52.138
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_2007320_02

Start Time:	2007-320T00:00:52.137	Stop Time:	2007-320T23:59:05.527
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007321_02

Start Time:	2007-321T00:00:05.527	Stop Time:	2007-321T23:59:06.917
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_2007322_02

Start Time:	2007-322T00:00:06.917	Stop Time:	2007-322T23:59:24.306
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007323_02

Start Time:	2007-323T00:00:09.306	Stop Time:	2007-323T23:59:10.696
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007324_02

Start Time:	2007-324T00:00:10.696	Stop Time:	2007-324T23:59:47.085
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007325_02

Start Time:	2007-325T00:00:32.085	Stop Time:	2007-325T23:59:49.475
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007326_02

Start Time:	2007-326T00:00:34.475	Stop Time:	2007-326T23:59:21.865
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007327_02

Start Time:	2007-327T00:00:06.865	Stop Time:	2007-327T23:59:16.254
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007328_02

Start Time:	2007-328T00:00:01.254	Stop Time:	2007-328T23:59:37.644
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007329_02

Start Time:	2007-329T00:00:22.644	Stop Time:	2007-329T23:59:31.034
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007330_02

Start Time:	2007-330T00:00:16.033	Stop Time:	2007-330T23:59:50.423
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007331_02

Start Time:	2007-331T00:00:35.423	Stop Time:	2007-331T23:59:16.813
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007332_02

Start Time:	2007-332T00:00:01.812	Stop Time:	2007-332T23:59:10.202
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_2007333_02

Start Time:	2007-333T00:00:10.202	Stop Time:	2007-333T23:59:11.592
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_2007334_02

Start Time:	2007-334T00:00:26.591	Stop Time:	2007-334T23:59:27.981
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007335_02

Start Time:	2007-335T00:00:27.981	Stop Time:	2007-335T23:59:29.371
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007336_02

Start Time:	2007-336T00:00:29.371	Stop Time:	2007-336T23:59:45.760
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007337_02

Start Time:	2007-337T00:00:30.760	Stop Time:	2007-337T23:59:42.150
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007338_02

Start Time:	2007-338T00:00:42.150	Stop Time:	2007-338T23:59:28.540
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007339_02

Start Time:	2007-339T00:00:13.539	Stop Time:	2007-339T23:59:28.929
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007340_02

Start Time:	2007-340T00:00:58.929	Stop Time:	2007-340T23:59:29.319
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_2007341_02

Start Time:	2007-341T00:00:59.318	Stop Time:	2007-341T23:59:31.708
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007342_02

Start Time:	2007-342T00:00:16.708	Stop Time:	2007-342T23:59:35.098
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007343_02

Start Time:	2007-343T00:00:20.098	Stop Time:	2007-343T23:59:51.488
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007344_02

Start Time:	2007-344T00:00:36.487	Stop Time:	2007-344T23:59:32.877
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007345_02

Start Time:	2007-345T00:00:17.877	Stop Time:	2007-345T23:59:48.267
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007346_02

Start Time:	2007-346T00:00:33.266	Stop Time:	2007-346T17:35:05.819
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007347_02

Start Time:	2007-347T01:10:21.626	Stop Time:	2007-347T08:04:32.451
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_2007348_02

Start Time:	2007-348T16:00:32.639	Stop Time:	2007-348T23:59:02.436
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_2007349_02

Start Time:	2007-349T00:00:32.435	Stop Time:	2007-349T23:59:02.825
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_2007350_02

Start Time:	2007-350T00:00:32.825	Stop Time:	2007-350T23:59:03.215
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007351_02

Start Time:	2007-351T00:00:33.214	Stop Time:	2007-351T23:59:49.604
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007352_02

Start Time:	2007-352T00:00:34.604	Stop Time:	2007-352T23:59:53.028
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007353_02

Start Time:	2007-353T00:00:38.027	Stop Time:	2007-353T23:59:34.417
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_2007354_02

Start Time:	2007-354T00:00:19.417	Stop Time:	2007-354T23:59:36.807
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007355_02

Start Time:	2007-355T00:00:21.807	Stop Time:	2007-355T23:59:37.197
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007356_02

Start Time:	2007-356T00:00:22.196	Stop Time:	2007-356T23:59:10.586
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007357_02

Start Time:	2007-357T00:00:10.586	Stop Time:	2007-357T23:59:11.976
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_2007358_02

Start Time:	2007-358T00:00:11.976	Stop Time:	2007-358T23:59:13.366
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007359_02

Start Time:	2007-359T00:00:13.365	Stop Time:	2007-359T23:59:30.755
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007360_02

Start Time:	2007-360T00:00:15.755	Stop Time:	2007-360T23:59:59.144
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_2007361_02

Start Time:	2007-361T00:01:41.144	Stop Time:	2007-361T23:59:30.534
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_2007362_02

Start Time:	2007-362T00:00:15.534	Stop Time:	2007-362T23:59:16.924
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007363_02

Start Time:	2007-363T00:00:16.923	Stop Time:	2007-363T23:59:02.314
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007364_02

Start Time:	2007-364T00:00:02.313	Stop Time:	2007-364T23:59:35.703
In an effort to make an INCA data product directly comparable to data products from the LEMMS and CHEMS telescopes, the images are collapsed in angle to form an image-integrated intensity. For each combination of energy (or in the case of INCA, time-of-flight (TOF)) from MIMI/INCA's high time resolution images, the original 32 x 32 image pixel intensity values in counts/(centimeters squaredsteradianseconds*keV) are averaged to a single intensity value. The energy ranges for the high time resolution range from high to low: (TOF id is the value in the TOF column in the file). There is no species differentiation. TOF id 0 = 55-90 keV TOF id 7 = 24-55 keV

IANGAVE0_T_2007365_02

Start Time:	2007-365T00:00:35.702	Stop Time:	2007-365T23:59:44.092
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

ICON LEGEND
For links to data holdings various icons are used to represent services or actions you can take. Those icons are:
	Order the volume (CD-ROM/DVD) containing the listed data. The volume will be mailed to you.	The volume (CD-ROM/DVD) contains some errors which are documented in an errata log.
	Launch a custom web browser for the resource.	Launch a map based browser for the resource.
	Toggle viewing into brief mode (shorter descriptions are displayed).	Toggle viewing into expanded mode (longer descriptions are displayed).
	Download the volume containing the listed data.

NEW RELEASES

More.....

PDS RESOURCES

Archive Planning Guide
      Individuals
      Missions
Data Dictionary Search
      Lookup Tool
      Document
PDS4 Standards Documents
PDS Subscription Service

PDS3 Standards

OTHER RESOURCES

ADS Search
Science Data Licenses

	Search For:

	in