INTEGRAL Galactic Plane Scanning
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