Revolution 1053b: Observation start 2011-05-31T01:50 = MJD 55712.077
Total Observation GTI = 56949 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 OSA9
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 176 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 88 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 301-2 186.666 -62.764 0.4 300.102 -0.029 62.7 0.47 134.0 4.5 0.35 12.7
Vela X-1 135.524 -40.552 0.6 263.054 +3.929 20.4 0.30 67.6 3.3 0.25 13.4
Cen X-3 170.296 -60.628 0.9 292.084 +0.328 12.8 0.38 33.9 0.0 0.00 0.0
1E 1145.1-6141 176.925 -61.970 2.2 295.519 -0.019 4.8 0.39 12.3 0.0 0.00 0.0
GX 304-1 195.280 -61.656 3.8 304.081 +1.194 3.1 0.46 6.7 0.0 0.00 0.0
IGR J12349-6434 188.763 -64.632 3.9 301.177 -1.816 2.4 0.37 6.5 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 l b A(cps) sigma
==================== ======== ======== ======== ======== ====== =====
H 0918-549 140.145 -55.198 275.852 -3.845 0.31 16.9
GX 304-1 195.338 -61.588 304.102 1.2475 0.18 10.1
4U 1323-62 201.643 -62.146 307.028 0.4556 0.11 6.0
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