INTEGRAL Galactic bulge Monitoring
Revolution 1386: Observation start 2014-02-20T12:51 = MJD 56708.536
Total Observation GTI = 12285 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1744-28 266.136 -28.741 0.3 0.044 +0.303 61.2 0.38 161.1 7.2 0.25 28.9 GX 1+4 263.005 -24.742 0.5 1.938 +4.800 32.8 0.44 75.4 0.0 0.00 0.0 GX 354-0 262.978 -33.841 1.0 354.292 -0.146 15.0 0.47 32.0 7.0 0.30 23.5 GRS 1758-258 270.311 -25.733 1.0 4.521 -1.363 12.8 0.43 29.8 9.3 0.27 34.7 GX 5-1 270.279 -25.075 1.2 5.078 -1.013 10.8 0.44 24.6 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.790 1.3 9.281 -6.088 17.1 0.78 22.0 6.1 0.46 13.2 4U 1700-377 255.995 -37.861 1.4 347.745 +2.158 14.1 0.68 20.7 4.2 0.42 10.1 GX 349+2 256.458 -36.427 2.3 349.112 +2.731 8.0 0.69 11.7 0.0 0.00 0.0 IGR J17544-2619 268.574 -26.345 3.1 3.209 -0.318 3.9 0.47 8.3 0.0 0.00 0.0 H 1820-303 275.950 -30.338 2.9 2.822 -7.927 5.3 0.58 9.0 0.0 0.00 0.0 GX 3+1 267.064 -26.561 4.4 2.333 +0.733 2.3 0.41 5.7 0.0 0.00 0.0 1A 1742-294 266.603 -29.595 0.0 359.527 -0.490 2.2 0.00 6.3 0.0 0.00 0.0 SGR J1745-29 266.504 -29.019 0.0 359.974 -0.117 2.1 0.00 5.9 0.0 0.00 0.0 3A 1822-371 276.412 -37.142 4.9 356.805 -11.283 4.2 0.83 5.1 0.0 0.00 0.0 SLX 1744-299_300 266.892 -30.086 0.0 359.237 -0.959 1.9 0.00 5.3 0.0 0.00 0.0 3A 1728-169 262.898 -16.856 4.7 8.585 +9.124 5.2 0.00 5.2 0.0 0.00 0.0 IGR J18193-2542 274.845 -25.806 5.0 6.422 -4.979 2.8 0.57 4.9 0.0 0.00 0.0 SLX 1735-269 264.552 -26.960 5.0 0.815 +2.433 2.0 0.00 5.0 2.2 0.26 8.5 GX 9+1 270.344 -20.472 5.2 9.108 +1.215 2.7 0.00 4.7 0.0 0.00 0.0 IGR J18027-2016 270.682 -20.302 0.0 9.412 +1.024 2.6 0.00 4.4 0.0 0.00 0.0 IGR J18048-1455 271.277 -14.841 6.8 14.453 +3.207 6.4 1.80 3.5 0.0 0.00 0.0 SAX J1808.4-3658 272.246 -36.969 5.4 355.444 -8.236 2.6 0.56 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 ~ 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 1742-294 266.529 -29.521 359.557 -0.396 8.9 0.27 33.2 1.6 0.15 10.4 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.27 3.6 0.2 0.15 1.4 4U 1722-30 261.888 -30.802 356.320 +2.298 2.8 0.38 7.4 0.9 0.25 3.6 GRO J1744-28 266.132 -28.746 0.038 +0.303 34.0 0.28 119.5 16.2 0.17 95.2 GRS 1758-258 270.303 -25.741 4.511 -1.361 7.3 1.27 5.7 2.1 0.66 3.2 GX 1+4 263.009 -24.746 1.937 +4.795 2.3 0.83 2.8 3.6 0.53 6.7 GX 3+1 266.986 -26.564 2.295 +0.792 55.8 0.46 121.8 6.3 0.23 27.0 GX 354-0 262.989 -33.835 354.302 -0.150 10.7 0.70 15.3 3.6 0.49 7.3 GX 5-1 270.284 -25.079 5.077 -1.019 125.9 1.96 64.2 18.0 1.00 18.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.4 0.34 4.1 0.5 0.19 2.4 SLX 1737-282 265.163 -28.297 359.971 +1.264 1.0 0.26 4.0 0.4 0.15 2.7 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.4 0.27 5.3 0.2 0.16 1.5 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.9 0.25 3.4 0.0 0.00 0.0 IGR J17544-2619 268.595 -26.333 3.230 -0.329 3.2 0.59 5.4 1.3 0.32 4.1 NEW SOURCE 271.468 -25.574 5.172 -2.194 16.6 2.73 6.1 2.2 1.55 1.4 NEW SOURCE 271.446 -26.204 4.611 -2.483 9.6 2.05 4.7 2.3 1.13 2.0 NEW SOURCE 266.381 -32.127 357.265 -1.644 0.4 0.32 1.2 0.6 0.20 3.1