INTEGRAL Galactic bulge Monitoring
Revolution 1267: Observation start 2013-02-28T14:27 = MJD 56351.603
Total Observation GTI = 12181 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 354-0 262.989 -33.839 0.8 354.298 -0.152 15.4 0.39 39.9 5.5 0.28 19.3 GRS 1758-258 270.316 -25.732 1.2 4.524 -1.367 9.5 0.36 26.2 6.8 0.26 25.8 Ginga 1826-24 277.352 -23.775 1.3 9.286 -6.065 13.0 0.56 23.4 4.5 0.39 11.6 Swift J174510.8-2624 266.291 -26.398 1.3 2.114 +1.410 8.2 0.35 23.6 5.1 0.26 19.3 XTE J1810-189 272.577 -19.085 1.8 11.345 +0.059 9.3 0.61 15.2 3.8 0.43 8.8 H 1820-303 275.927 -30.356 2.2 2.797 -7.918 6.0 0.49 12.2 0.0 0.00 0.0 KS 1741-293 266.194 -29.350 2.1 359.551 -0.059 3.9 0.31 12.7 1.4 0.24 5.9 SLX 1744-299_300 266.877 -30.009 3.3 359.297 -0.908 2.4 0.31 7.8 1.3 0.24 5.3 H 1702-429 256.511 -43.100 0.0 343.812 -1.326 14.0 0.00 7.8 4.8 1.21 3.9 MXB 1730-335 263.261 -33.317 3.5 354.860 -0.057 2.8 0.38 7.4 0.0 0.00 0.0 3A 1822-371 276.465 -37.025 3.8 356.931 -11.270 4.3 0.65 6.7 0.0 0.00 0.0 GX 1+4 263.024 -24.755 4.3 1.937 +4.779 2.5 0.43 5.9 0.0 0.00 0.0 GX 349+2 256.493 -36.426 3.7 349.129 +2.710 4.3 0.62 6.9 0.0 0.00 0.0 GX 3+1 266.974 -26.535 0.0 2.314 +0.815 2.2 0.00 6.4 0.0 0.00 0.0 GX 9+1 270.401 -20.493 4.0 9.116 +1.158 3.1 0.49 6.2 0.0 0.00 0.0 GX 17+2 273.948 -14.029 4.2 16.412 +1.331 19.7 3.28 6.0 0.0 0.00 0.0 SLX 1735-269 264.652 -27.092 5.7 0.751 +2.287 1.5 0.35 4.3 0.8 0.26 3.3 4U 1722-30 261.859 -30.758 4.6 356.342 +2.343 2.0 0.36 5.4 0.0 0.00 0.0 Swift J1753.7-2544 268.382 -25.746 5.3 3.639 +0.134 1.6 0.34 4.6 1.1 0.00 4.2 XTE J1752-223 268.039 -22.448 0.0 6.321 +2.080 2.0 0.00 4.6 0.0 0.00 0.0 H 1745-203 267.326 -20.351 5.8 7.788 +3.720 2.1 0.00 4.2 0.0 0.00 0.0 V2400 Oph 258.129 -24.224 5.8 359.873 +8.769 2.2 0.00 4.2 0.0 0.00 0.0 XTE J1739-285 264.917 -28.536 7.0 359.654 +1.320 1.1 0.31 3.4 0.0 0.00 0.0 GX 13+1 273.649 -17.136 5.3 13.543 +0.102 4.3 0.92 4.6 0.0 0.00 0.0 IGR J17091-3624 257.298 -36.374 6.5 349.559 +2.222 2.1 0.57 3.7 1.4 0.00 3.6 Swift J175759.9-2246 269.457 -22.677 0.0 6.784 +0.833 1.6 0.00 3.7 0.0 0.00 0.0 Swift J1749.4-2807 267.253 -28.097 6.7 1.104 -0.202 1.2 0.00 3.6 0.0 0.00 0.0 HETE J1900.1-2455 285.018 -24.932 7.0 11.287 -12.862 42.4 12.31 3.4 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 1742-294 266.516 -29.519 359.552 -0.386 10.8 0.25 43.1 2.0 0.13 15.2 4U 1722-30 261.888 -30.802 356.320 +2.298 2.3 0.57 4.1 0.4 0.38 1.2 GRS 1734-292 264.367 -29.142 358.883 +1.404 1.2 0.30 4.0 0.3 0.16 2.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.6 0.77 3.4 1.2 0.33 3.8 GX 3+1 266.982 -26.567 2.290 +0.793 52.1 0.42 123.9 5.3 0.19 28.4 GX 354-0 262.989 -33.835 354.302 -0.150 12.6 1.08 11.6 3.6 0.75 4.8 GX 5-1 270.284 -25.076 5.080 -1.017 104.8 1.29 81.5 4.9 0.48 10.3 MXB 1730-335 263.350 -33.388 354.841 -0.158 20.0 0.86 23.3 4.2 0.56 7.5 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.2 0.24 4.9 0.5 0.13 4.1 XTE J1739-285 264.974 -28.497 359.713 +1.298 9.7 0.29 33.0 0.7 0.15 4.8 Swift J174510.8-2624 266.284 -26.412 2.099 +1.407 2.7 0.41 6.5 1.2 0.19 6.2 NEW SOURCE 269.567 -25.914 4.031 -0.872 2.9 0.57 5.0 0.0 0.00 0.0 KS 1741-293 266.215 -29.350 359.560 -0.074 0.9 0.25 3.6 0.7 0.13 5.0