INTEGRAL Galactic bulge Monitoring
Revolution 1079: Observation start 2011-08-15T07:41 = MJD 55788.321
Total Observation GTI = 12261 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 5-1 270.281 -25.092 1.0 5.065 -1.022 11.8 0.37 32.2 0.0 0.00 0.0 GX 354-0 262.997 -33.839 1.0 354.302 -0.158 12.0 0.38 31.3 3.5 0.29 12.0 Ginga 1826-24 277.372 -23.809 1.6 9.263 -6.097 12.4 0.68 18.2 5.3 0.49 10.8 IGR J17498-2921 267.486 -29.322 1.5 0.158 -1.008 6.6 0.34 19.4 4.5 0.27 16.5 1E 1740.7-2942 265.990 -29.736 1.7 359.129 -0.110 5.7 0.34 16.6 4.4 0.28 16.0 GX 349+2 256.482 -36.438 1.8 349.114 +2.709 9.8 0.62 15.8 0.0 0.00 0.0 GRS 1758-258 270.311 -25.738 1.9 4.517 -1.366 5.2 0.36 14.3 3.6 0.28 13.0 GX 1+4 262.984 -24.749 2.1 1.922 +4.812 5.0 0.38 13.2 0.0 0.00 0.0 GX 9+1 270.390 -20.516 2.4 9.091 +1.156 5.2 0.48 10.9 0.0 0.00 0.0 4U 1722-30 261.850 -30.827 2.8 356.281 +2.312 3.4 0.36 9.5 1.8 0.28 6.4 GX 17+2 273.952 -14.027 3.8 16.416 +1.328 15.2 2.27 6.7 0.0 0.00 0.0 OAO 1657-415 255.237 -41.637 3.6 344.400 +0.311 11.0 1.56 7.1 0.0 0.00 0.0 H 1820-303 275.922 -30.342 4.2 2.807 -7.908 3.3 0.54 6.0 0.0 0.00 0.0 GX 3+1 267.018 -26.606 3.7 2.274 +0.746 2.4 0.36 6.9 0.0 0.00 0.0 IGR J17091-3624 257.281 -36.474 4.5 349.471 +2.173 3.3 0.60 5.5 0.0 0.00 0.0 SLX 1735-269 264.514 -26.938 6.4 0.816 +2.474 1.3 0.34 3.8 0.0 0.00 0.0 3A 1822-371 276.373 -37.104 5.7 356.826 -11.238 3.3 0.00 4.3 0.0 0.00 0.0 MXB 1730-335 263.466 -33.428 0.0 354.860 -0.261 1.5 0.00 4.1 0.0 0.00 0.0 GRS 1741.9-2853 266.308 -28.896 6.7 359.990 +0.094 1.1 0.32 3.6 0.0 0.00 0.0 Swift J165534.1-4426 253.983 -44.524 6.1 341.567 -0.763 30.1 7.51 4.0 0.0 0.00 0.0 Oph Cluster 258.007 -23.325 5.5 0.552 +9.377 2.1 0.47 4.5 0.0 0.00 0.0 IGR J17448-3232 266.212 -32.465 0.0 356.902 -1.699 1.3 0.00 3.9 0.0 0.00 0.0 GX 13+1 273.619 -17.164 0.0 13.505 +0.114 3.5 0.00 3.9 0.0 0.00 0.0 1RXS J165424.7-29541 253.606 -29.853 6.4 352.873 +8.639 2.3 0.00 3.8 0.0 0.00 0.0 V1223 Sgr 283.711 -31.155 6.8 4.949 -14.313 8.3 2.34 3.6 0.0 0.00 0.0 IGR J17254-3257 261.333 -32.881 0.0 354.331 +1.530 1.3 0.00 3.6 0.0 0.00 0.0 4U 1735-444 264.844 -44.502 5.7 346.047 -7.083 17.1 4.00 4.3 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 6.7 0.23 29.4 1.1 0.13 8.3 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.1 0.21 5.1 0.8 0.13 6.3 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.2 0.23 5.3 0.3 0.14 2.2 4U 1722-30 261.888 -30.802 356.320 +2.298 1.3 0.35 3.7 0.5 0.24 1.9 GX 1+4 263.009 -24.746 1.937 +4.795 1.7 0.54 3.2 0.7 0.34 2.0 GX 3+1 266.991 -26.553 2.307 +0.794 47.2 0.35 133.3 4.7 0.18 26.3 GX 354-0 262.989 -33.835 354.302 -0.150 10.9 0.81 13.5 2.8 0.62 4.4 GX 5-1 270.287 -25.082 5.076 -1.022 105.5 1.56 67.5 15.5 0.78 19.9 SLX 1735-269 264.571 -26.994 0.796 +2.400 0.8 0.26 3.2 0.3 0.15 1.7 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.8 0.23 16.2 0.6 0.14 4.6 IGR J17498-2921 267.486 -29.318 0.161 -1.006 1.9 0.25 7.4 1.0 0.15 6.6 NEW SOURCE 268.962 -23.432 5.903 +0.849 10.6 1.79 5.9 0.0 0.00 0.0 NEW SOURCE 268.805 -27.397 2.406 -1.028 1.8 0.37 4.8 0.3 0.20 1.4