INTEGRAL Galactic bulge Monitoring
Revolution 1849: Observation start 2017-08-10T11:25 = MJD 57975.476
Total Observation GTI = 26855 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17464-3213 266.565 -32.234 0.5 357.255 -1.833 38.9 0.44 88.7 16.3 0.20 80.9 GX 354-0 262.980 -33.835 0.6 354.298 -0.144 35.9 0.58 62.1 9.6 0.25 38.2 1E 1740.7-2942 265.985 -29.744 0.7 359.120 -0.110 20.1 0.44 45.6 10.7 0.21 52.0 GRS 1716-249 259.897 -25.027 0.8 0.131 +6.990 23.1 0.55 42.0 11.1 0.24 46.9 4U 1700-377 255.978 -37.837 0.8 347.756 +2.183 42.0 1.01 41.8 10.9 0.42 25.9 GRS 1758-258 270.299 -25.739 0.9 4.510 -1.357 17.0 0.49 34.9 7.5 0.22 34.8 OAO 1657-415 255.197 -41.670 1.5 344.355 +0.315 43.8 2.35 18.7 9.1 0.91 10.0 GX 17+2 274.029 -14.037 1.9 16.442 +1.258 35.0 2.42 14.5 0.0 0.00 0.0 H 1820-303 275.937 -30.329 2.4 2.824 -7.913 7.1 0.65 11.0 0.0 0.00 0.0 GX 5-1 270.341 -25.056 2.9 5.123 -1.052 4.1 0.45 9.0 0.0 0.00 0.0 GX 1+4 263.020 -24.728 2.3 1.957 +4.796 5.2 0.46 11.4 0.0 0.00 0.0 SLX 1735-269 264.545 -26.957 3.2 0.814 +2.440 3.7 0.46 8.1 2.1 0.21 10.3 1A 1743-288 266.715 -28.865 3.2 0.202 -0.195 3.6 0.45 8.0 1.2 0.21 5.6 GX 9+1 270.491 -20.498 3.7 9.153 +1.082 4.3 0.62 7.0 0.0 0.00 0.0 MXB 1730-335 263.381 -33.396 0.0 354.848 -0.184 3.7 0.00 7.0 0.0 0.00 0.0 3A 1822-371 276.469 -37.017 4.1 356.940 -11.270 5.8 0.94 6.2 0.0 0.00 0.0 SAX J1712.6-3739 258.251 -37.669 3.6 348.965 +0.842 6.3 0.90 7.0 2.0 0.37 5.3 XTE J1812-182 273.109 -18.113 3.9 12.439 +0.085 5.4 0.82 6.6 0.0 0.00 0.0 PKS 1830-211 278.311 -21.090 4.3 12.095 -5.637 5.7 0.00 5.8 0.0 0.00 0.0 GX 349+2 256.442 -36.525 4.5 349.026 +2.683 5.0 0.91 5.5 0.0 0.00 0.0 SLX 1746-331 267.452 -33.123 5.1 356.878 -2.931 2.3 0.48 4.8 0.0 0.00 0.0 IGR J17200-3116 260.004 -31.370 5.4 354.941 +3.313 2.5 0.55 4.5 0.0 0.00 0.0 XTE J1752-223 268.064 -22.326 5.6 6.438 +2.121 2.3 0.52 4.4 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 1742-294 266.530 -29.511 359.566 -0.392 0.9 0.15 5.9 0.0 0.00 0.0 1E 1740.7-2942 265.992 -29.742 359.125 -0.114 0.6 0.14 4.1 0.0 0.00 0.0 GX 3+1 266.986 -26.558 2.299 +0.795 5.6 0.17 33.0 0.7 0.14 4.6 GX 5-1 270.286 -25.078 5.079 -1.019 78.1 1.43 54.7 2.0 0.80 2.5 IGR J17464-3213 266.570 -32.228 357.262 -1.834 1.3 0.32 4.0 0.0 0.00 0.0 MXB 1730-335 263.350 -33.388 354.841 -0.158 5.7 0.78 7.3 0.0 0.00 0.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 0.5 0.14 3.6 0.0 0.00 0.0 GRS 1716-249 259.908 -25.010 0.151 +6.992 5.0 0.99 5.1 1.6 0.97 1.6 NEW SOURCE 270.365 -25.279 4.940 -1.180 4.6 1.19 3.9 0.0 0.00 0.0 NEW SOURCE 266.105 -22.074 5.720 +3.807 5.0 1.31 3.8 0.0 0.00 0.0 NEW SOURCE 265.717 -22.220 5.408 +4.037 4.3 1.13 3.8 0.0 0.00 0.0 IGR J17536-2339 268.456 -23.659 5.472 +1.134 3.4 1.04 3.3 0.0 0.00 0.0