Revolution 2311b: Observation start 2020-12-22T03:25 = MJD 59205.143
Total Observation GTI = 73463 seconds
ISGRI
![2311b_isgri_mosa1.jpg](2311b_isgri_mosa1.jpg)
![2311b_isgri_mosa2.jpg](2311b_isgri_mosa2.jpg)
ISGRI significance mosaic images. Top: ISGRI 18-40 keV. Bottom: 40-100 keV
Sources detected > 10σ in each band are marked on the image. The table below lists the fitted position, and statistical positional uncertainty in arcmin returned by the mosaic step of OSA10.2
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 cps ) where available.
ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)
Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig
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GX 301-2 186.651 -62.773 1.0 300.096 -0.038 4.8 0.15 32.0 1.2 0.16 7.5
Circinus Galaxy 213.263 -65.344 2.6 311.313 -3.809 1.1 0.11 10.3 0.5 0.12 4.3
4U 1323-62 201.629 -62.122 2.3 307.020 +0.471 1.2 0.10 11.5 0.5 0.11 4.5
IGR J11435-6109 176.033 -61.094 4.0 294.888 +0.722 1.9 0.30 6.2 0.0 0.00 0.0
NGC 4945 196.389 -49.457 3.9 305.289 +13.350 1.7 0.27 6.5 1.2 0.28 4.3
JEM-X Detected Sources 3-10 keV
Sources were detected in the 3-10 keV image > 5σ and are listed in the table below. Fluxes are extracted at the known catalogue position of the source (i.e. no fitting of the source position is done), with j_ima_src_locator
in 3-10 keV energy band.
/
Source Name RA dec A(cps) sigma
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