INTEGRAL Galactic bulge Monitoring
Revolution 1511: Observation start 2015-02-24T23:52 = MJD 57077.995
Total Observation GTI = 12100 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 1RXS J180408.9-34205 271.028 -34.336 0.7 357.305 -6.114 23.1 0.48 48.4 10.4 0.30 34.7 Ginga 1826-24 277.374 -23.791 1.0 9.281 -6.091 21.3 0.68 31.4 8.7 0.41 21.4 MXB 1746-20 267.211 -20.356 1.1 7.729 +3.810 15.9 0.55 29.2 0.0 0.00 0.0 GRS 1758-258 270.298 -25.744 1.1 4.506 -1.358 12.0 0.43 27.9 7.5 0.27 27.8 GRO J1750-27 267.260 -26.633 1.2 2.362 +0.546 9.8 0.38 26.0 1.5 0.24 6.0 GX 1+4 263.012 -24.745 1.1 1.939 +4.793 12.2 0.46 26.5 0.0 0.00 0.0 GX 5-1 270.282 -25.077 1.7 5.078 -1.016 7.4 0.44 16.7 1.1 0.27 3.9 KS 1741-293 266.222 -29.343 2.9 359.570 -0.075 3.1 0.35 9.0 1.8 0.23 7.8 IGR J17252-3616 261.304 -36.271 2.7 351.510 -0.351 5.1 0.53 9.7 0.0 0.00 0.0 H 1820-303 275.912 -30.340 3.3 2.805 -7.899 4.3 0.55 7.8 0.0 0.00 0.0 SLX 1744-299_300 266.874 -30.021 3.0 359.285 -0.912 3.0 0.34 8.7 1.4 0.23 6.0 GX 17+2 274.048 -14.000 3.0 16.484 +1.259 25.9 2.93 8.8 0.0 0.00 0.0 GX 349+2 256.446 -36.445 2.9 349.091 +2.729 6.1 0.67 9.1 0.0 0.00 0.0 SLX 1735-269 264.612 -26.985 3.7 0.823 +2.375 2.6 0.38 6.9 1.7 0.25 6.8 4U 1722-30 261.907 -30.836 4.0 356.301 +2.266 2.5 0.40 6.3 1.1 0.26 4.2 1E 1740.7-2942 265.967 -29.753 3.5 359.104 -0.101 2.6 0.35 7.3 1.8 0.24 7.5 SAX J1806.5-2215 271.677 -22.241 3.9 8.176 -0.735 3.4 0.52 6.6 0.0 0.00 0.0 H 1702-429 256.586 -43.047 4.2 343.887 -1.338 14.7 2.47 6.0 0.0 0.00 0.0 IGR J17204-3554 260.062 -35.956 4.6 351.201 +0.654 2.9 0.00 5.4 0.0 0.00 0.0 GRS 1747-312 267.717 -31.293 4.0 358.567 -2.189 2.4 0.38 6.4 1.5 0.25 6.1 GX 3+1 266.862 -26.535 0.0 2.263 +0.901 1.9 0.00 5.0 0.0 0.00 0.0 MXB 1730-335 263.266 -33.372 4.7 354.816 -0.091 2.1 0.41 5.3 0.0 0.00 0.0 GRS 1739-278 265.630 -27.677 5.1 0.715 +1.240 1.7 0.36 4.9 1.1 0.24 4.5 AX J1736.4-2910 264.202 -29.158 5.7 358.793 +1.517 1.5 0.34 4.3 0.0 0.00 0.0 IGR J17586-2129 269.736 -21.403 5.4 8.017 +1.245 2.3 0.49 4.6 0.0 0.00 0.0 1RXS J175721.2-30440 269.462 -30.694 5.9 359.839 -3.177 1.6 0.00 4.1 0.0 0.00 0.0 GX 9+1 270.396 -20.559 5.6 9.056 +1.129 2.3 0.54 4.4 0.0 0.00 0.0 GX 354-0 262.952 -33.797 0.0 354.317 -0.104 1.7 0.00 4.1 0.0 0.00 0.0 3A 1822-371 276.414 -37.031 5.8 356.908 -11.237 3.5 0.84 4.2 0.0 0.00 0.0 1A 1743-288 266.685 -28.838 0.0 0.211 -0.158 1.3 0.00 3.9 0.0 0.00 0.0 3A 1728-169 262.916 -16.972 5.2 8.495 +9.047 4.2 0.89 4.7 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 1742-294 266.528 -29.519 359.558 -0.395 11.0 0.25 44.4 2.2 0.14 15.6 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.3 0.24 5.3 0.8 0.14 5.2 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.24 4.0 0.2 0.14 1.2 4U 1722-30 261.888 -30.802 356.320 +2.298 3.3 0.48 6.8 0.8 0.33 2.3 CONFUSED ID 266.523 -29.515 359.559 -0.389 11.1 0.25 45.0 2.3 0.14 15.8 GRO J1750-27 267.314 -26.661 2.363 +0.491 3.2 0.35 9.2 3.3 0.19 17.3 GX 1+4 263.009 -24.746 1.937 +4.795 2.7 0.80 3.4 2.1 0.53 3.9 GX 3+1 266.973 -26.564 2.288 +0.802 36.5 0.36 102.1 3.9 0.18 21.5 GX 354-0 262.990 -33.827 354.309 -0.147 25.8 1.14 22.5 5.0 0.85 5.8 GX 5-1 270.280 -25.071 5.082 -1.011 152.0 1.47 103.7 18.3 0.65 28.1 MXB 1730-335 263.363 -33.388 354.846 -0.168 10.5 0.80 13.1 2.5 0.56 4.4 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.7 0.30 5.6 0.5 0.18 2.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.25 7.2 0.8 0.15 5.1 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.7 0.24 7.2 0.4 0.14 2.8 NEW SOURCE 266.823 -22.799 5.444 +2.863 11.1 1.95 5.7 1.7 1.10 1.5 NEW SOURCE 269.221 -23.376 6.070 +0.671 10.5 2.04 5.2 2.0 1.18 1.7 NEW SOURCE 273.190 -28.105 3.690 -4.758 6.8 1.38 4.9 2.0 1.07 1.9 NEW SOURCE 270.792 -23.946 6.291 -0.861 18.7 3.41 5.5 0.0 0.00 0.0 KS 1741-293 266.219 -29.349 359.563 -0.076 0.8 0.24 3.3 0.6 0.14 4.5