INTEGRAL Galactic bulge Monitoring
Revolution 1279: Observation start 2013-04-06T00:03 = MJD 56388.003
Total Observation GTI = 12460 seconds
ISGRI
ISGRI significance mosaic images. Left: 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
OSA9, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 210 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 104 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. 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 354-0 262.990 -33.827 0.7 354.309 -0.146 20.7 0.41 50.1 6.9 0.29 23.6 GRS 1758-258 270.304 -25.747 1.2 4.506 -1.365 9.7 0.38 25.2 6.9 0.27 26.0 IGR J18245-2452 276.141 -24.863 1.4 7.806 -5.581 12.1 0.56 21.6 6.1 0.37 16.3 Ginga 1826-24 277.366 -23.783 1.4 9.284 -6.080 15.3 0.72 21.3 5.9 0.47 12.5 GX 349+2 256.450 -36.421 2.0 349.112 +2.740 9.3 0.66 14.0 0.0 0.00 0.0 GX 1+4 263.007 -24.773 1.8 1.913 +4.781 5.3 0.35 15.1 0.0 0.00 0.0 Swift J174510.8-2624 266.286 -26.399 1.8 2.111 +1.413 5.1 0.33 15.6 3.4 0.24 14.1 KS 1741-293 266.253 -29.350 2.5 359.578 -0.102 3.4 0.33 10.5 1.6 0.23 6.7 OAO 1657-415 255.184 -41.650 2.6 344.365 +0.334 27.3 2.67 10.2 0.0 0.00 0.0 H 1820-303 275.873 -30.310 3.3 2.816 -7.855 4.3 0.55 7.8 0.0 0.00 0.0 GX 3+1 267.019 -26.560 2.4 2.314 +0.769 3.5 0.32 10.9 0.0 0.00 0.0 SAX J1806.5-2215 271.615 -22.252 3.0 8.139 -0.690 3.8 0.44 8.7 1.7 0.30 5.7 SLX 1744-299_300 266.842 -29.976 2.8 359.309 -0.865 3.4 0.36 9.4 0.0 0.00 0.0 IGR J17091-3624 257.263 -36.387 2.9 349.532 +2.237 5.7 0.63 9.1 4.5 0.43 10.5 3A 1822-371 276.507 -37.156 3.0 356.825 -11.357 6.9 0.80 8.6 0.0 0.00 0.0 GX 9+1 270.405 -20.506 0.0 9.106 +1.149 3.5 0.00 7.0 0.0 0.00 0.0 SLX 1735-269 264.560 -26.989 3.4 0.796 +2.411 2.8 0.36 7.7 1.6 0.25 6.5 XTE J1739-285 265.004 -28.533 3.5 359.697 +1.257 2.7 0.36 7.4 1.1 0.25 4.6 XTE J1810-189 272.540 -19.058 3.6 11.352 +0.103 4.5 0.64 7.1 0.0 0.00 0.0 GX 5-1 270.262 -25.022 4.3 5.117 -0.973 2.1 0.36 5.8 0.0 0.00 0.0 4U 1700-377 255.995 -37.858 0.0 347.747 +2.159 4.3 0.00 5.1 0.0 0.00 0.0 NEW SOURCE 249.747 -22.491 4.5 356.530 +15.949 10.5 1.82 5.5 0.0 0.00 0.0 NEW SOURCE 275.389 -19.623 4.5 12.134 -2.530 3.8 0.68 5.6 0.0 0.00 0.0 NEW SOURCE 256.678 -40.341 3.7 346.090 +0.237 8.4 1.22 6.9 0.0 0.00 0.0 NEW SOURCE 260.508 -26.427 3.9 359.279 +5.748 2.5 0.39 6.4 0.0 0.00 0.0 NEW SOURCE 266.203 -17.007 3.9 10.122 +6.348 3.8 0.59 6.4 0.0 0.00 0.0 NEW SOURCE 265.616 -41.964 4.1 348.524 -6.242 7.8 1.26 6.2 0.0 0.00 0.0 NEW SOURCE 257.024 -21.932 3.9 1.178 +10.922 3.2 0.49 6.6 0.0 0.00 0.0 NEW SOURCE 276.863 -24.538 4.3 8.398 -6.015 3.4 0.57 5.9 0.0 0.00 0.0 NEW SOURCE 252.429 -23.915 5.4 356.968 +13.134 3.9 0.85 4.6 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 ~ 235 cps [J1], 249 cps [J2]); B = 10-25 keV (1 Crab ~ 74 cps [J1], 70 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 15.7 0.52 30.3 2.4 0.27 8.9 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 2.8 0.48 5.9 0.4 0.25 1.6 4U 1722-30 261.888 -30.802 356.320 +2.298 5.7 0.93 6.2 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 6.8 1.49 4.6 2.4 0.70 3.5 GX 3+1 266.983 -26.568 2.290 +0.792 114.5 0.66 174.4 12.5 0.29 43.3 GX 354-0 262.989 -33.835 354.302 -0.150 24.4 3.61 6.8 9.1 2.99 3.0 GX 5-1 270.298 -25.069 5.092 -1.024 197.8 2.15 91.9 8.3 0.85 9.7 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.2 0.45 4.7 0.7 0.24 2.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.8 0.56 5.0 0.7 0.31 2.4 XTE J1739-285 264.975 -28.496 359.714 +1.298 2.6 0.46 5.6 0.6 0.24 2.3 Swift J174510.8-2624 266.278 -26.404 2.103 +1.416 4.1 0.51 8.0 1.1 0.25 4.4 NEW SOURCE 270.895 -26.690 3.946 -2.291 8.3 1.50 5.6 0.0 0.00 0.0 KS 1741-293 266.214 -29.332 359.576 -0.064 2.3 0.47 5.0 1.0 0.26 3.7 NEW SOURCE 268.161 -23.359 5.593 +1.519 8.3 1.77 4.7 0.0 0.00 0.0