INTEGRAL Galactic bulge Monitoring
Revolution 0409: Observation start 2006-02-17T21:11 = MJD 53783.883
Total Observation GTI = 12011 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 1700-377 255.992 -37.842 0.4 347.759 +2.171 72.5 0.73 100.0 20.7 0.55 37.6 GRS 1758-258 270.288 -25.743 0.9 4.502 -1.350 10.8 0.31 34.5 5.8 0.25 22.9 GX 5-1 270.280 -25.089 1.0 5.067 -1.020 10.5 0.33 31.5 0.0 0.00 0.0 Ginga 1826-24 277.355 -23.788 1.0 9.276 -6.073 18.2 0.61 29.6 7.1 0.48 14.7 GX 1+4 263.006 -24.747 1.0 1.935 +4.797 10.4 0.35 29.8 0.0 0.00 0.0 1A 1742-294 266.515 -29.504 1.2 359.565 -0.377 7.1 0.29 24.9 2.2 0.24 9.3 XTE J1817-330 274.419 -33.021 1.6 359.811 -7.987 8.1 0.44 18.3 3.5 0.35 9.9 OAO 1657-415 255.189 -41.667 1.7 344.354 +0.321 23.0 1.43 16.2 7.3 1.05 7.0 GX 354-0 262.987 -33.831 1.9 354.305 -0.146 5.6 0.39 14.6 0.0 0.00 0.0 GX 349+2 256.455 -36.410 2.0 349.123 +2.744 7.9 0.60 13.3 0.0 0.00 0.0 H 1820-303 275.916 -30.356 2.0 2.792 -7.910 6.2 0.46 13.6 0.0 0.00 0.0 3A 1822-371 276.437 -37.119 2.6 356.835 -11.291 7.2 0.70 10.4 0.0 0.00 0.0 GX 17+2 274.036 -14.026 2.6 16.455 +1.257 21.3 2.11 10.1 0.0 0.00 0.0 GX 9+1 270.381 -20.516 3.5 9.086 +1.163 3.4 0.46 7.3 0.0 0.00 0.0 IGR J17252-3616 261.302 -36.320 3.0 351.468 -0.378 4.0 0.45 8.7 0.0 0.00 0.0 SLX 1744-299_300 266.878 -30.046 3.0 359.266 -0.928 2.7 0.32 8.6 0.0 0.00 0.0 XB 1832-330 278.953 -32.981 3.6 1.548 -11.382 4.2 0.60 7.0 0.0 0.00 0.0 4U 1722-30 261.901 -30.822 3.9 356.309 +2.278 2.5 0.38 6.5 1.5 0.31 4.8 SLX 1735-269 264.538 -26.946 4.2 0.821 +2.451 2.1 0.35 6.0 0.0 0.00 0.0 SGR J1745-29 266.495 -29.002 0.0 359.985 -0.102 1.7 0.00 6.1 0.0 0.00 0.0 GX 3+1 267.013 -26.630 3.8 2.250 +0.737 2.2 0.32 6.6 0.0 0.00 0.0 3A 1728-169 262.920 -16.921 5.6 8.540 +9.070 3.0 0.69 4.4 0.0 0.00 0.0 GX 13+1 273.660 -17.135 4.1 13.549 +0.093 4.7 0.75 6.2 0.0 0.00 0.0 4U 1735-444 264.852 -44.482 4.8 346.068 -7.077 20.3 3.89 5.2 0.0 0.00 0.0 IGR J17331-2406 263.338 -24.210 5.9 2.552 +4.833 1.6 0.39 4.1 0.0 0.00 0.0
JEM-X
JEM-X1 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 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 1.9 0.28 7.0 0.9 0.17 5.1 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.4 0.29 4.7 0.0 0.00 0.0 4U 1722-30 261.888 -30.802 356.320 +2.298 1.7 0.51 3.2 0.7 0.32 2.1 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.6 0.34 4.8 0.3 0.22 1.3 GX 3+1 266.971 -26.563 2.289 +0.803 20.3 0.43 47.4 2.2 0.22 9.8 GX 354-0 262.985 -33.831 354.303 -0.145 21.9 1.16 18.8 3.4 0.82 4.2 GX 5-1 270.288 -25.079 5.079 -1.021 124.6 1.94 64.3 14.3 0.88 16.3 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.1 0.36 3.0 0.3 0.22 1.4 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.2 0.28 4.3 0.3 0.17 2.0 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.1 0.28 3.8 0.0 0.00 0.0 XTE J1739-285 264.991 -28.494 359.724 +1.287 6.4 0.29 22.0 1.0 0.17 5.9 NEW SOURCE 271.515 -26.106 4.728 -2.490 9.4 1.57 6.0 0.9 0.80 1.1 NEW SOURCE 271.207 -24.206 6.250 -1.319 23.7 4.10 5.8 3.8 2.27 1.7 NEW SOURCE 266.096 -23.347 4.627 +3.151 7.3 1.54 4.7 0.0 0.00 0.0 NEW SOURCE 267.957 -23.726 5.183 +1.494 8.4 1.48 5.7 0.0 0.00 0.0 NEW SOURCE 266.300 -23.583 4.523 +2.868 6.2 1.16 5.4 1.0 0.72 1.4 NEW SOURCE 270.144 -24.728 5.319 -0.734 8.4 1.69 5.0 1.3 0.84 1.5