Revolution 2161: Observation start 2019-11-17T21:24 = MJD 58804.893
Total Observation GTI = 38678 seconds
ISGRI
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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GRS 1915+105 288.797 +10.944 0.8 45.364 -0.218 6.9 0.16 43.8 0.0 0.00 0.0
XTE J1855-026 283.910 -2.601 4.3 31.095 -2.120 1.8 0.31 5.8 0.0 0.00 0.0
IGR J18450-0435 281.317 -4.586 3.6 28.147 -0.721 3.3 0.47 7.0 0.0 0.00 0.0
EXO 1846-031 282.355 -3.018 4.0 30.016 -0.927 2.2 0.36 6.3 0.0 0.00 0.0
AX J1847.6-0156 281.875 -1.859 4.5 30.829 +0.029 1.8 0.00 5.6 0.0 0.00 0.0
JEM-X
JEM-X1 and JEM-X2 significance mosaic images in 3-10 keV energy band.
Note: Sources labelled 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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