INTEGRAL Galactic bulge Monitoring
Revolution 1667: Observation start 2016-04-13T13:06 = MJD 57491.547
Total Observation GTI = 12453 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.991 -37.849 0.6 347.753 +2.168 69.7 1.04 67.2 21.0 0.57 36.6 GRS 1758-258 270.302 -25.738 1.1 4.512 -1.359 14.8 0.51 29.1 8.9 0.29 30.3 GX 5-1 270.287 -25.085 1.1 5.073 -1.024 13.8 0.50 27.9 0.0 0.00 0.0 GX 354-0 262.976 -33.831 2.3 354.300 -0.139 5.8 0.50 11.5 0.0 0.00 0.0 H 1820-303 275.891 -30.348 2.5 2.789 -7.886 7.8 0.74 10.6 0.0 0.00 0.0 GX 349+2 256.534 -36.426 3.1 349.149 +2.683 7.6 0.92 8.3 0.0 0.00 0.0 SLX 1735-269 264.498 -27.064 2.7 0.702 +2.418 4.4 0.45 9.7 1.8 0.28 6.6 SAX J1806.5-2215 271.623 -22.204 3.3 8.184 -0.674 4.6 0.58 7.9 2.2 0.35 6.4 IGR J17464-3213 266.619 -32.170 3.3 357.334 -1.839 3.7 0.48 7.9 1.3 0.27 4.7 GX 9+1 270.340 -20.554 4.7 9.034 +1.177 3.6 0.68 5.3 0.0 0.00 0.0 SLX 1744-299_300 266.821 -30.110 4.3 359.185 -0.919 2.9 0.00 5.8 0.0 0.00 0.0 3A 1822-371 276.454 -37.049 4.9 356.905 -11.273 5.2 1.03 5.1 0.0 0.00 0.0 Ginga 1826-24 277.267 -23.757 4.7 9.266 -5.987 4.8 0.90 5.3 0.0 0.00 0.0 1A 1743-288 266.714 -28.795 0.0 0.261 -0.157 2.2 0.00 5.1 0.0 0.00 0.0 GX 1+4 262.972 -24.762 4.2 1.905 +4.814 3.0 0.50 6.0 0.0 0.00 0.0 IGR J17488-2338 267.112 -23.639 5.6 4.860 +2.203 2.2 0.50 4.4 0.0 0.00 0.0 Oph Cluster 258.133 -23.343 4.5 0.605 +9.273 3.8 0.69 5.5 0.0 0.00 0.0 GRS 1734-292 264.416 -29.128 4.3 358.918 +1.375 2.7 0.46 5.8 0.0 0.00 0.0 GRS 1739-278 265.661 -27.713 4.9 0.699 +1.198 2.2 0.43 5.1 0.0 0.00 0.0 IGR J17098-3628 257.394 -36.510 0.0 349.496 +2.079 3.6 0.00 4.8 0.0 0.00 0.0 GX 17+2 273.929 -14.033 5.2 16.399 +1.345 14.5 3.06 4.7 0.0 0.00 0.0 IGR J18193-2542 274.851 -25.800 5.3 6.430 -4.981 3.4 0.00 4.7 0.0 0.00 0.0 IGR J17507-2856 267.671 -28.939 5.5 0.570 -0.950 2.0 0.45 4.5 0.0 0.00 0.0 IGR J17513-2011 267.807 -20.223 6.1 8.128 +3.397 2.5 0.64 4.0 0.0 0.00 0.0 PKS 1830-211 278.476 -21.110 5.8 12.147 -5.783 5.3 0.00 4.2 0.0 0.00 0.0 IGR J18179-1621 274.388 -16.366 6.2 14.557 -0.153 6.0 1.52 3.9 0.0 0.00 0.0 4U 1722-30 261.759 -30.792 6.1 356.266 +2.396 1.9 0.00 4.0 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 1742-294 266.523 -29.515 359.559 -0.389 5.4 0.38 14.1 0.8 0.26 3.3 4U 1722-30 261.888 -30.802 356.320 +2.298 3.6 0.62 5.8 0.7 0.49 1.5 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 2.9 0.36 8.0 0.4 0.25 1.6 GX 3+1 266.983 -26.564 2.294 +0.794 18.4 0.51 35.9 1.7 0.31 5.4 GX 354-0 262.989 -33.835 354.302 -0.150 16.1 1.51 10.6 1.9 1.44 1.3 GX 5-1 270.284 -25.079 5.077 -1.019 159.1 2.67 59.6 24.0 1.46 16.4 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.3 0.36 3.6 0.6 0.26 2.3 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.4 0.40 3.4 0.0 0.00 0.0 NEW SOURCE 270.012 -24.885 5.124 -0.708 10.3 2.07 5.0 0.0 0.00 0.0