INTEGRAL Galactic bulge Monitoring
Revolution 1346: Observation start 2013-10-21T17:35 = MJD 56586.733
Total Observation GTI = 12238 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== Ginga 1826-24 277.366 -23.794 1.1 9.274 -6.085 20.0 0.71 28.3 7.8 0.48 16.3 GX 1+4 262.994 -24.753 1.1 1.923 +4.802 10.1 0.36 28.2 0.0 0.00 0.0 GRS 1758-258 270.283 -25.741 1.2 4.501 -1.346 9.0 0.36 24.8 6.6 0.26 25.2 OAO 1657-415 255.202 -41.651 1.8 344.372 +0.324 17.7 1.14 15.5 6.1 0.78 7.9 H 1820-303 275.953 -30.336 2.2 2.824 -7.929 5.9 0.48 12.3 0.0 0.00 0.0 MAXI J1828-249 277.252 -25.018 2.1 8.129 -6.547 8.0 0.62 12.9 4.8 0.42 11.5 MXB 1730-335 263.343 -33.387 2.3 354.838 -0.152 3.7 0.31 11.9 0.0 0.00 0.0 1E 1740.7-2942 265.969 -29.739 2.6 359.117 -0.096 3.4 0.33 10.2 2.4 0.25 9.8 GX 349+2 256.452 -36.410 2.7 349.122 +2.746 5.1 0.52 9.9 0.0 0.00 0.0 3A 1822-371 276.455 -37.138 3.0 356.823 -11.312 5.5 0.64 8.6 0.0 0.00 0.0 Swift J1734.5-3027 263.599 -30.444 3.0 357.428 +1.263 2.7 0.32 8.5 1.1 0.24 4.5 GX 354-0 262.937 -33.811 4.2 354.299 -0.101 2.3 0.38 6.1 0.0 0.00 0.0 GX 3+1 267.063 -26.596 3.6 2.303 +0.716 2.4 0.33 7.1 0.0 0.00 0.0 SLX 1735-269 264.497 -27.033 3.5 0.728 +2.436 2.3 0.32 7.2 1.1 0.24 4.6 GX 5-1 270.402 -25.074 0.0 5.135 -1.109 2.6 0.00 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.922 -30.071 4.4 359.264 -0.974 1.8 0.31 5.7 0.0 0.00 0.0 1A 1742-294 266.463 -29.581 5.6 359.476 -0.379 1.5 0.00 4.4 0.0 0.00 0.0 XTE J1720-318 260.039 -31.735 5.7 354.657 +3.080 1.6 0.38 4.3 0.0 0.00 0.0 GX 9+1 270.359 -20.424 6.4 9.156 +1.226 1.9 0.49 3.8 0.0 0.00 0.0 XTE J1751-305 267.811 -30.635 6.3 359.174 -1.921 1.3 0.00 3.8 0.0 0.00 0.0 4U 1722-30 261.811 -30.829 5.0 356.260 +2.338 1.8 0.36 4.9 0.0 0.00 0.0 Swift J174535.5-2901 266.364 -29.005 0.0 359.922 -0.006 1.2 0.00 3.7 0.0 0.00 0.0 GRS 1734-292 264.293 -29.166 0.0 358.829 +1.446 1.1 0.00 3.6 0.9 0.23 3.7 XB 1832-330 278.963 -32.916 6.8 1.611 -11.362 2.3 0.66 3.6 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 1742-294 266.521 -29.512 359.562 -0.386 6.5 0.23 28.1 1.1 0.13 9.0 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 0.5 0.22 2.3 0.4 0.12 3.3 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.24 3.9 0.2 0.13 1.8 4U 1722-30 261.876 -30.794 356.320 +2.311 15.4 0.36 42.2 2.2 0.20 11.0 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.0 0.24 8.4 0.4 0.14 2.7 GX 3+1 266.984 -26.561 2.297 +0.795 47.1 0.50 94.2 4.9 0.25 19.9 GX 354-0 262.991 -33.834 354.304 -0.151 18.9 0.54 34.8 3.2 0.31 10.2 GX 5-1 270.292 -25.082 5.078 -1.026 66.6 3.02 22.0 0.0 0.00 0.0 MXB 1730-335 263.350 -33.388 354.841 -0.158 15.1 0.44 34.7 2.9 0.25 11.5 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.8 0.35 5.1 0.6 0.19 3.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.3 0.23 10.2 0.3 0.13 2.6 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.9 0.23 3.9 0.3 0.13 2.2 Swift J1734.5-3027 263.615 -30.387 357.482 +1.283 1.4 0.24 5.8 0.4 0.14 3.0 NEW SOURCE 270.648 -26.324 4.156 -1.918 3.7 1.20 3.1 0.0 0.00 0.0 NEW SOURCE 268.983 -25.222 4.365 -0.070 4.9 1.16 4.2 0.0 0.00 0.0