INTEGRAL Galactic bulge Monitoring
Revolution 1333: Observation start 2013-09-13T15:20 = MJD 56548.639
Total Observation GTI = 10893 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 354-0 262.994 -33.833 0.7 354.306 -0.153 22.3 0.41 53.7 7.1 0.28 25.0 4U 1700-377 255.974 -37.865 1.0 347.732 +2.169 24.2 0.73 33.3 7.0 0.47 14.8 GX 5-1 270.279 -25.079 1.1 5.075 -1.014 12.7 0.45 28.5 0.0 0.00 0.0 GRS 1758-258 270.307 -25.760 1.2 4.496 -1.374 10.8 0.45 23.9 7.8 0.31 25.6 Ginga 1826-24 277.373 -23.803 1.2 9.269 -6.095 18.2 0.73 24.9 8.0 0.47 17.1 GX 1+4 263.007 -24.746 1.3 1.936 +4.796 10.2 0.45 22.7 0.0 0.00 0.0 IGR J17464-3213 266.593 -32.252 2.7 357.252 -1.863 3.8 0.39 9.8 2.4 0.28 8.5 OAO 1657-415 255.170 -41.620 2.7 344.382 +0.361 12.3 1.28 9.6 5.4 0.82 6.6 H 1820-303 275.973 -30.385 2.6 2.788 -7.966 5.5 0.54 10.2 0.0 0.00 0.0 IGR J17252-3616 261.324 -36.283 2.8 351.509 -0.371 4.2 0.45 9.4 0.0 0.00 0.0 3A 1822-371 276.423 -37.078 3.0 356.867 -11.263 6.3 0.71 8.8 0.0 0.00 0.0 GX 349+2 256.449 -36.418 2.8 349.114 +2.743 5.8 0.63 9.3 0.0 0.00 0.0 SLX 1735-269 264.586 -27.013 2.9 0.787 +2.379 3.5 0.40 8.9 1.3 0.28 4.8 GX 3+1 266.910 -26.542 3.3 2.278 +0.861 3.1 0.40 7.8 0.0 0.00 0.0 GX 9+1 270.354 -20.567 4.4 9.030 +1.160 3.4 0.59 5.7 0.0 0.00 0.0 IGR J17404-3655 265.063 -37.026 0.0 352.521 -3.292 2.5 0.00 5.2 0.0 0.00 0.0 GRS 1734-292 264.312 -29.129 3.8 358.869 +1.452 2.2 0.34 6.6 0.0 0.00 0.0 MXB 1730-335 263.341 -33.494 0.0 354.748 -0.210 2.1 0.00 5.1 0.0 0.00 0.0 1A 1742-294 266.636 -29.522 4.8 359.605 -0.477 1.7 0.32 5.2 0.0 0.00 0.0 Oph Cluster 258.069 -23.290 5.0 0.615 +9.351 2.7 0.56 4.9 0.0 0.00 0.0 GRS 1741.9-2853 266.256 -28.989 4.6 359.887 +0.083 1.8 0.33 5.4 0.0 0.00 0.0 IGR J17353-3539 263.773 -35.707 5.3 353.080 -1.709 2.0 0.00 4.6 0.0 0.00 0.0 XTE J1752-223 267.961 -22.392 5.2 6.333 +2.170 2.2 0.45 4.8 0.0 0.00 0.0 SLX 1744-299_300 266.763 -30.049 5.1 359.211 -0.844 1.6 0.33 4.8 0.0 0.00 0.0 SAX J1818.6-1703 274.662 -17.018 5.5 14.108 -0.694 5.7 1.28 4.4 0.0 0.00 0.0 GX 17+2 273.908 -13.998 6.0 16.421 +1.379 22.9 5.67 4.0 0.0 0.00 0.0 NEW SOURCE 267.601 -34.862 4.5 355.443 -3.925 2.4 0.43 5.6 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 1742-294 266.523 -29.515 359.559 -0.389 11.1 0.24 45.9 1.9 0.13 14.0 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.0 0.22 4.3 0.2 0.13 1.7 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.25 3.6 0.2 0.14 1.4 4U 1722-30 261.888 -30.802 356.320 +2.298 4.0 0.40 10.0 0.9 0.26 3.4 GX 3+1 266.973 -26.563 2.290 +0.802 54.2 0.50 108.8 6.3 0.24 26.1 GX 354-0 262.989 -33.835 354.302 -0.150 14.2 0.67 21.4 5.4 0.44 12.2 GX 5-1 270.284 -25.093 5.065 -1.025 110.8 2.52 44.0 20.9 1.34 15.6 IGR J17464-3213 266.567 -32.229 357.260 -1.832 1.0 0.25 4.2 0.7 0.16 4.1 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 0.9 0.22 4.2 0.3 0.13 2.2 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.8 0.24 3.4 0.2 0.13 1.1 NEW SOURCE 266.306 -23.930 4.229 +2.683 6.1 1.36 4.4 0.0 0.00 0.0 NEW SOURCE 264.207 -24.273 2.925 +4.131 4.1 1.17 3.5 0.0 0.00 0.0 NEW SOURCE 270.918 -26.009 4.550 -1.975 7.0 2.04 3.4 0.0 0.00 0.0