INTEGRAL Galactic bulge Monitoring
Revolution 1226: Observation start 2012-10-27T15:03 = MJD 56227.628
Total Observation GTI = 10738 seconds
IBIS/ISGRI
IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 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.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 and NEW SOURCEs < 6σ towards the border of the image may be spurious. IBIS/ISGRI Detected Sources 18-40 keV (A) and 40-100 keV (B)
Source Name RA dec +/- l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== Swift J174510.8-2624 266.298 -26.403 0.4 2.113 +1.402 50.9 0.38 135.7 20.9 0.28 75.4 4U 1700-377 255.977 -37.845 0.7 347.749 +2.179 41.6 0.79 53.0 10.5 0.53 19.9 GX 5-1 270.296 -25.085 1.1 5.078 -1.030 11.8 0.44 26.7 0.0 0.00 0.0 GX 1+4 263.006 -24.734 1.3 1.945 +4.803 10.6 0.45 23.5 0.0 0.00 0.0 Ginga 1826-24 277.365 -23.797 1.3 9.272 -6.085 15.4 0.70 21.9 5.9 0.47 12.6 IGR J17464-3213 266.543 -32.222 2.0 357.256 -1.811 5.8 0.42 13.6 3.7 0.30 12.3 GRS 1758-258 270.338 -25.741 2.1 4.526 -1.389 5.7 0.44 13.1 3.6 0.31 11.7 3A 1822-371 276.448 -37.121 2.3 356.837 -11.299 8.5 0.72 11.8 0.0 0.00 0.0 IGR J17091-3624 257.287 -36.400 2.3 349.533 +2.214 7.1 0.60 11.7 3.5 0.41 8.4 H 1820-303 275.939 -30.397 2.8 2.764 -7.945 4.8 0.52 9.3 1.6 0.35 4.6 GX 349+2 256.452 -36.426 2.2 349.109 +2.736 9.0 0.73 12.3 0.0 0.00 0.0 4U 1722-30 261.913 -30.818 2.4 356.319 +2.271 4.7 0.43 11.0 2.0 0.29 6.8 1E 1740.7-2942 265.995 -29.743 2.6 359.126 -0.117 3.7 0.37 10.0 2.0 0.28 7.1 GX 3+1 266.974 -26.520 3.3 2.326 +0.824 2.9 0.38 7.8 0.0 0.00 0.0 SLX 1735-269 264.581 -26.995 3.4 0.800 +2.392 2.9 0.38 7.6 1.8 0.27 6.5 SAX J1806.5-2215 271.616 -22.237 3.6 8.152 -0.684 3.6 0.50 7.1 0.0 0.00 0.0 OAO 1657-415 255.177 -41.673 4.7 344.344 +0.325 9.1 0.00 5.3 0.0 0.00 0.0 GRS 1747-312 267.554 -31.288 4.8 358.500 -2.066 2.0 0.39 5.1 0.0 0.00 0.0 IGR J17354-3255 263.966 -32.848 5.2 355.574 -0.300 2.0 0.00 4.7 0.0 0.00 0.0 GX 9+1 270.399 -20.511 4.5 9.099 +1.151 3.5 0.62 5.6 0.0 0.00 0.0 IGR J17252-3616 261.150 -36.270 5.9 351.441 -0.248 2.1 0.00 4.1 0.0 0.00 0.0 3A 1728-169 263.022 -16.941 6.5 8.576 +8.978 3.6 0.96 3.7 0.0 0.00 0.0 SAX J1752.3-3138 268.108 -31.580 5.1 358.489 -2.621 1.9 0.39 4.9 0.0 0.00 0.0 1A 1742-294 266.502 -29.500 0.0 359.563 -0.365 1.5 0.00 3.7 0.0 0.00 0.0 XTE J1710-281 257.551 -28.174 6.0 356.323 +6.897 2.0 0.50 4.0 0.0 0.00 0.0 XTE J1739-285 264.909 -28.505 0.0 359.676 +1.343 1.4 0.00 3.5 0.9 0.30 3.0 SLX 1744-299_300 266.969 -29.959 5.8 359.380 -0.951 1.6 0.38 4.2 0.0 0.00 0.0 IGR J18027-2016 270.698 -20.235 6.0 9.477 +1.043 2.5 0.61 4.1 0.0 0.00 0.0 NEW SOURCE 259.074 -23.605 4.3 0.886 +8.414 3.1 0.52 5.9 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band 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 ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]). NOTES: 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. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1;
NEW SOURCEs < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.
JEM-X1+2 Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== ===== 1A 1742-294 266.511 -29.495 359.571 -0.370 8.4 0.31 27.4 1.3 0.15 8.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.2 0.29 4.0 0.5 0.15 3.0 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.7 0.30 9.0 0.5 0.16 3.0 GX 3+1 266.978 -26.567 2.288 +0.796 44.3 0.59 75.6 5.4 0.27 19.9 GX 354-0 262.989 -33.835 354.302 -0.150 11.1 0.73 15.3 2.1 0.43 5.0 GX 5-1 270.284 -25.078 5.078 -1.018 131.5 2.36 55.7 24.4 1.27 19.2 IGR J17464-3213 266.567 -32.229 357.260 -1.832 0.8 0.32 2.4 0.6 0.17 3.4 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.8 0.47 6.0 0.6 0.24 2.4 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.7 0.29 5.8 0.3 0.15 2.2 Swift J174510.8-2624 266.306 -26.403 2.117 +1.395 44.9 0.60 74.7 10.4 0.29 36.2 NEW SOURCE 266.321 -24.774 3.514 +2.232 4.5 1.02 4.4 1.2 0.52 2.2 NEW SOURCE 268.972 -24.014 5.404 +0.547 12.0 3.16 3.8 0.0 0.00 0.0 NEW SOURCE 266.575 -25.273 3.207 +1.777 3.5 0.83 4.2 0.0 0.00 0.0 NEW SOURCE 265.291 -24.671 3.112 +3.083 4.2 1.14 3.7 0.8 0.62 1.2 NEW SOURCE 270.783 -26.646 3.936 -2.182 4.5 1.16 3.9 0.6 0.57 1.0