Revolution 1622: Observation start 2015-12-15T16:52 = MJD 57371.704
Total Observation GTI = 61010 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 OSA10.1
, 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 301-2 186.654 -62.770 0.6 300.097 -0.035 10.8 0.17 65.0 1.4 0.11 12.8
1E 1145.1-6141 176.877 -61.946 1.0 295.491 -0.001 4.3 0.15 29.7 1.2 0.10 12.2
Cen X-3 170.329 -60.634 1.3 292.101 +0.329 3.4 0.15 22.5 0.8 0.10 7.3
4U 1323-62 201.562 -62.136 2.9 306.987 +0.461 2.6 0.29 8.9 1.3 0.19 6.8
4U 1036-56 159.402 -56.835 3.1 285.372 +1.403 2.4 0.28 8.5 0.9 0.19 5.1
IGR J12349-6434 188.841 -64.562 3.7 301.206 -1.744 1.1 0.16 6.9 0.0 0.00 0.0
1H 1255-567 193.495 -57.110 4.4 303.279 +5.760 1.4 0.00 5.7 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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