INTEGRAL Galactic Bulge Monitoring Revolution 0531: Observation start 2007-02-17 = MJD 54148
Total Observation GTI = 25402 seconds
ISGRI
ISGRI significance mosaic images. Left: ISGRI 18-40 keV. Right: 40-100 keVSources 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
OSA7
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 cps ) where available.NOTES: The table is constructed from the
isgri_mosa_res.fits
file - fluxes in the mosaic output are known to be systematically ~10% lower than in the ScW light-curves (see known issues). The systematic noise increases towards the edge of the field of view andNEW
sources < 6σ towards the border of the image may be spurious.
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 1+4 263.013 -24.746 0.5 1.939 +4.792 16.2 0.22 72.9 0.0 0.00 0.0 GRS 1758-258 270.297 -25.746 0.7 4.504 -1.359 11.1 0.23 48.2 8.0 0.19 42.8 1E 1740.7-2942 265.978 -29.750 0.7 359.112 -0.108 9.4 0.20 46.6 6.9 0.17 40.6 Ginga 1826-24 277.359 -23.801 0.8 9.265 -6.083 17.0 0.39 43.2 6.9 0.31 22.5 4U 1700-377 255.990 -37.850 0.8 347.752 +2.168 17.7 0.45 39.5 5.9 0.35 17.0 GX 5-1 270.285 -25.088 1.0 5.070 -1.023 7.3 0.23 31.6 0.0 0.00 0.0 GX 354-0 262.989 -33.819 1.1 354.315 -0.142 6.1 0.23 27.1 0.0 0.00 0.0 GX 349+2 256.426 -36.428 1.2 349.095 +2.752 9.2 0.38 24.2 0.0 0.00 0.0 H 1820-303 275.903 -30.375 1.3 2.769 -7.908 7.0 0.32 22.2 0.0 0.00 0.0 OAO 1657-415 255.196 -41.659 1.5 344.363 +0.322 17.4 0.88 19.8 6.5 0.65 10.0 3A 1822-371 276.464 -37.106 1.5 356.856 -11.305 8.1 0.41 19.5 0.0 0.00 0.0 GX 3+1 266.978 -26.575 1.8 2.282 +0.792 3.2 0.21 15.1 0.0 0.00 0.0 4U 1722-30 261.881 -30.808 2.0 356.311 +2.300 3.2 0.23 13.5 1.3 0.19 6.6 GX 9+1 270.374 -20.549 2.4 9.054 +1.153 3.2 0.30 10.9 0.0 0.00 0.0 SLX 1744-299_300 266.866 -30.005 2.3 359.295 -0.898 2.3 0.20 11.4 0.9 0.17 5.7 GRS 1741.9-2853 266.330 -28.923 2.7 359.977 +0.063 2.0 0.20 9.8 0.7 0.17 4.0 SLX 1735-269 264.522 -27.032 2.8 0.741 +2.417 2.1 0.22 9.3 1.0 0.19 5.5 GX 17+2 274.001 -14.019 2.9 16.445 +1.290 14.4 1.58 9.1 0.0 0.00 0.0 1A 1742-294 266.468 -29.423 4.5 359.613 -0.300 1.1 0.19 5.5 0.0 0.00 0.0 GX 13+1 273.711 -17.161 4.3 13.550 +0.038 3.2 0.55 5.8 0.0 0.00 0.0 SLX 1737-282 265.156 -28.305 5.1 359.961 +1.264 1.0 0.21 4.9 0.0 0.00 0.0 3A 1728-169 262.934 -17.037 4.6 8.448 +8.998 2.5 0.47 5.4 0.0 0.00 0.0 Oph Cluster 258.179 -23.375 5.0 0.603 +9.219 1.5 0.31 4.9 0.0 0.00 0.0 H 1702-429 256.584 -43.011 4.9 343.915 -1.315 5.9 1.17 5.0 0.0 0.00 0.0 IGR J17195-4100 259.759 -40.988 5.2 346.940 -2.034 2.5 0.52 4.8 0.0 0.00 0.0 XTE J1710-281 257.582 -28.146 0.0 356.361 +6.891 1.2 0.00 4.1 0.0 0.00 0.0JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.Note: Sources labelled were detected with 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
mosaic_spec
, in two bands: A = 3-10 keV (1 Crab ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).NOTE: The object marked as SLX 1744-299_300 is used to indicate two low-mass x-ray binaries separated by 2.7 arcminutes, SLX 1744-299 and SLX 1744-300; the position for SLX 1744-299 is used, although it can not be ruled out that SLX 1744-300 may dominate the emission some of the time.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 20.7 1.25 5.4 0.79 1A 1742-294 266.523 -29.515 359.559 -0.389 1.4 0.22 0.5 0.14 GX 3+1 266.983 -26.564 2.294 +0.794 30.9 0.40 4.1 0.21 GX 5-1 270.284 -25.079 5.077 -1.019 77.2 1.47 6.6 0.63 IGR J17454-2703 266.329 -27.039 1.584 +1.046 2.7 0.45 0.4 0.28
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