INTEGRAL Galactic bulge Monitoring
Revolution 1280: Observation start 2013-04-09T16:36 = MJD 56391.692
Total Observation GTI = 10973 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 354-0 262.985 -33.838 0.7 354.298 -0.149 22.3 0.47 46.9 6.4 0.32 20.0 4U 1700-377 255.979 -37.835 0.9 347.758 +2.184 33.5 0.98 34.1 10.9 0.63 17.2 GRS 1758-258 270.296 -25.745 1.1 4.504 -1.357 10.2 0.38 26.8 6.4 0.26 24.5 Ginga 1826-24 277.388 -23.787 1.2 9.290 -6.100 14.2 0.56 25.1 7.5 0.37 20.2 IGR J18245-2452 276.154 -24.856 1.7 7.818 -5.588 9.7 0.59 16.6 4.4 0.38 11.5 Swift J174510.8-2624 266.311 -26.408 1.8 2.114 +1.389 5.8 0.38 15.3 4.1 0.27 15.4 GX 1+4 263.006 -24.749 2.0 1.932 +4.796 6.0 0.43 13.9 0.0 0.00 0.0 KS 1741-293 266.217 -29.325 2.0 359.583 -0.062 5.1 0.38 13.4 1.9 0.27 7.1 SAX J1806.5-2215 271.612 -22.165 2.9 8.214 -0.646 3.9 0.42 9.1 0.0 0.00 0.0 GX 5-1 270.290 -25.062 3.3 5.095 -1.014 3.2 0.41 7.8 0.0 0.00 0.0 GX 3+1 267.010 -26.537 2.8 2.329 +0.787 3.4 0.37 9.2 0.0 0.00 0.0 H 1820-303 275.969 -30.408 3.0 2.766 -7.974 4.7 0.53 8.8 0.0 0.00 0.0 GX 17+2 273.971 -14.016 3.8 16.434 +1.317 11.9 1.80 6.6 0.0 0.00 0.0 IGR J18027-2016 270.649 -20.273 0.0 9.421 +1.065 3.5 0.00 6.7 0.0 0.00 0.0 3A 1822-371 276.454 -37.058 3.4 356.896 -11.277 5.7 0.76 7.5 0.0 0.00 0.0 IGR J17091-3624 257.254 -36.351 4.4 349.557 +2.264 4.9 0.86 5.7 4.5 0.57 7.9 GX 9+1 270.310 -20.603 3.6 8.978 +1.177 3.4 0.48 7.2 0.0 0.00 0.0 SLX 1735-269 264.521 -27.013 4.1 0.756 +2.428 2.6 0.43 6.2 1.7 0.29 5.8 XTE J1739-285 265.076 -28.479 3.9 359.776 +1.232 2.4 0.37 6.5 0.0 0.00 0.0 SLX 1744-299_300 266.934 -29.978 4.6 359.349 -0.934 2.1 0.39 5.4 0.0 0.00 0.0 1RXS J182129.0-13164 275.355 -13.204 3.9 17.786 +0.516 18.6 2.84 6.6 0.0 0.00 0.0 GX 349+2 256.435 -36.428 4.8 349.100 +2.746 4.6 0.89 5.1 0.0 0.00 0.0 NEW SOURCE 276.525 -13.275 3.5 18.257 -0.523 19.5 2.76 7.2 2.8 0.43 6.6 NEW SOURCE 276.232 -40.797 4.1 353.366 -12.719 9.4 1.52 6.2 16.5 2.36 7.0 NEW SOURCE 259.966 -13.948 3.6 9.544 +13.068 11.5 1.59 7.1 0.0 0.00 0.0 NEW SOURCE 269.601 -20.498 3.8 8.739 +1.806 3.3 0.49 6.7 0.0 0.00 0.0 NEW SOURCE 278.059 -17.863 3.6 14.869 -3.956 7.0 0.97 7.1 0.0 0.00 0.0 NEW SOURCE 260.611 -25.071 4.2 0.460 +6.431 2.7 0.45 6.0 0.0 0.00 0.0 NEW SOURCE 258.190 -40.631 5.4 346.541 -0.861 7.7 1.72 4.6 0.0 0.00 0.0 NEW SOURCE 263.628 -34.062 4.6 354.400 -0.719 2.7 0.50 5.5 0.0 0.00 0.0 NEW SOURCE 280.921 -33.456 4.6 1.806 -13.077 4.8 0.89 5.4 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 ~ 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 -29.527 359.549 -0.395 16.8 0.69 24.5 2.8 0.34 8.3 4U 1722-30 261.888 -30.802 356.320 +2.298 8.1 2.02 4.0 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.4 1.11 2.2 1.8 0.48 3.8 GX 3+1 266.981 -26.567 2.290 +0.794 115.6 0.71 161.8 12.8 0.30 43.0 GX 5-1 270.285 -25.088 5.070 -1.024 231.5 1.61 143.6 16.3 0.60 27.4 SLX 1735-269 264.571 -26.994 0.796 +2.400 3.4 0.65 5.2 0.9 0.31 2.7 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 4.3 0.78 5.5 0.8 0.38 2.1 NEW SOURCE 271.441 -24.725 5.902 -1.758 16.3 2.20 7.4 1.1 0.90 1.2 Swift J174510.8-2624 266.289 -26.408 2.104 +1.406 1.5 0.63 2.3 1.1 0.29 3.8 KS 1741-293 266.206 -29.345 359.560 -0.065 2.0 0.66 3.1 0.9 0.34 2.6