INTEGRAL Galactic bulge Monitoring
Revolution 1668: Observation start 2016-04-16T00:50 = MJD 57494.035
Total Observation GTI = 12589 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 5-1 270.280 -25.074 0.9 5.080 -1.012 16.8 0.48 35.2 1.5 0.29 5.4 GRS 1758-258 270.311 -25.741 1.0 4.514 -1.367 13.5 0.45 30.2 9.1 0.27 33.9 GX 354-0 262.999 -33.865 2.7 354.281 -0.174 5.0 0.51 9.7 1.2 0.31 4.1 GX 9+1 270.393 -20.537 3.6 9.074 +1.143 4.2 0.59 7.1 0.0 0.00 0.0 IGR J17091-3624 257.233 -36.412 3.7 349.497 +2.241 5.3 0.77 6.9 2.7 0.43 6.2 SLX 1735-269 264.589 -26.970 3.2 0.825 +2.400 3.7 0.45 8.2 2.1 0.28 7.6 H 1820-303 275.891 -30.359 4.0 2.779 -7.892 4.1 0.66 6.2 0.0 0.00 0.0 GX 1+4 262.991 -24.728 3.4 1.943 +4.819 3.5 0.47 7.4 0.0 0.00 0.0 Oph Cluster 258.078 -23.319 4.3 0.595 +9.327 3.7 0.63 5.8 0.0 0.00 0.0 XTE J1814-338 273.493 -33.693 4.5 358.849 -7.611 3.5 0.64 5.6 0.0 0.00 0.0 GX 349+2 256.474 -36.486 4.2 349.072 +2.686 4.9 0.82 5.9 0.0 0.00 0.0 KS 1741-293 266.280 -29.335 4.3 359.603 -0.115 2.4 0.41 5.9 1.5 0.25 5.9 IGR J18027-2016 270.713 -20.277 0.0 9.448 +1.010 3.4 0.00 5.5 0.0 0.00 0.0 SAX J1750.8-2900 267.604 -29.087 4.6 0.413 -0.976 2.5 0.45 5.4 0.0 0.00 0.0 1RXS J180408.9-34205 271.112 -34.319 0.0 357.354 -6.167 2.8 0.00 5.0 0.0 0.00 0.0 4U 1722-30 261.971 -30.801 4.7 356.360 +2.240 2.4 0.46 5.3 0.0 0.00 0.0 IGR J17473-2721 266.740 -27.436 5.4 1.435 +0.527 1.9 0.00 4.6 0.0 0.00 0.0 XTE J1716-389 258.991 -38.830 6.3 348.362 -0.307 3.8 0.98 3.8 0.0 0.00 0.0 3A 1728-169 262.904 -16.969 4.9 8.491 +9.058 4.7 0.94 5.0 0.0 0.00 0.0 IGR J17375-3022 264.270 -30.379 5.8 357.794 +0.811 1.9 0.00 4.2 0.0 0.00 0.0 Swift J174540.7-2900 266.477 -28.978 4.6 359.997 -0.076 2.6 0.47 5.5 0.0 0.00 0.0 OAO 1657-415 255.191 -41.580 0.0 344.423 +0.373 12.8 0.00 3.9 6.3 0.00 3.4 IGR J18048-1455 271.222 -14.955 5.5 14.328 +3.197 7.8 1.75 4.5 0.0 0.00 0.0 IGR J17464-3213 266.484 -32.146 6.1 357.294 -1.728 1.8 0.45 4.0 2.5 0.27 9.1 H 1705-250 257.168 -25.067 6.9 358.665 +8.992 2.3 0.68 3.5 1.4 0.00 3.5 XMMSL1 J171900.4-353 259.870 -35.481 6.6 351.501 +1.053 2.4 0.65 3.7 0.0 0.00 0.0 SLX 1737-282 265.153 -28.335 6.7 359.934 +1.250 1.4 0.00 3.6 1.3 0.25 5.2 IGR J17252-3616 261.217 -36.237 0.0 351.499 -0.274 2.4 0.00 3.5 0.0 0.00 0.0 SAX J1806.5-2215 271.638 -22.213 7.0 8.183 -0.690 2.0 0.58 3.4 1.5 0.00 4.3 GX 17+2 273.995 -14.111 0.0 16.362 +1.251 8.9 0.00 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 1742-294 266.523 -29.515 359.559 -0.389 5.1 0.36 14.4 0.9 0.27 3.5 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.3 0.34 4.0 0.0 0.00 0.0 GX 3+1 266.974 -26.561 2.291 +0.802 11.6 0.43 27.0 1.2 0.30 4.2 GX 354-0 262.989 -33.835 354.302 -0.150 12.9 2.69 4.8 5.1 2.61 1.9 GX 5-1 270.283 -25.081 5.075 -1.018 112.3 1.56 71.7 20.5 0.87 23.4 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.9 0.36 5.2 0.5 0.29 1.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.1 0.37 8.5 0.7 0.28 2.6 NEW SOURCE 271.445 -26.867 4.032 -2.805 5.3 1.20 4.4 0.0 0.00 0.0 NEW SOURCE 270.343 -25.814 4.465 -1.429 4.6 1.05 4.4 0.8 0.66 1.2 NEW SOURCE 267.780 -23.121 5.620 +1.942 6.3 1.71 3.7 0.0 0.00 0.0 NEW SOURCE 268.013 -22.166 6.552 +2.244 13.9 3.23 4.3 3.3 2.39 1.4 NEW SOURCE 268.507 -22.444 6.544 +1.708 11.6 3.39 3.4 0.0 0.00 0.0 NEW SOURCE 266.098 -23.002 4.923 +3.329 5.2 1.39 3.8 0.0 0.00 0.0 NEW SOURCE 269.635 -23.738 5.947 +0.162 7.3 2.04 3.6 0.0 0.00 0.0