INTEGRAL Galactic bulge Monitoring
Revolution 0417: Observation start 2006-03-15T09:54 = MJD 53809.413
Total Observation GTI = 12067 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 5-1 270.279 -25.082 0.7 5.072 -1.016 16.5 0.32 51.9 0.0 0.00 0.0 GRS 1758-258 270.291 -25.752 0.9 4.495 -1.357 10.9 0.32 33.5 6.9 0.26 26.3 GX 1+4 263.007 -24.749 0.9 1.933 +4.795 11.5 0.32 35.7 0.0 0.00 0.0 Ginga 1826-24 277.352 -23.796 1.0 9.266 -6.075 17.7 0.59 29.9 6.3 0.46 13.9 1A 1742-294 266.515 -29.515 1.4 359.556 -0.383 5.8 0.29 20.4 2.4 0.24 10.1 GX 354-0 262.993 -33.823 1.6 354.314 -0.147 6.4 0.37 17.2 0.0 0.00 0.0 GX 349+2 256.422 -36.435 2.1 349.088 +2.750 7.5 0.57 13.1 0.0 0.00 0.0 H 1820-303 275.921 -30.342 1.8 2.806 -7.906 7.4 0.48 15.5 0.0 0.00 0.0 XTE J1817-330 274.457 -33.013 2.0 359.832 -8.012 5.6 0.42 13.4 2.9 0.32 8.9 3A 1822-371 276.468 -37.081 2.7 356.881 -11.297 5.7 0.60 9.6 0.0 0.00 0.0 GX 3+1 267.001 -26.576 2.7 2.292 +0.774 3.3 0.34 9.8 0.0 0.00 0.0 GX 9+1 270.428 -20.534 3.3 9.093 +1.116 3.8 0.48 7.9 0.0 0.00 0.0 XTE J1739-285 264.980 -28.425 3.6 359.777 +1.332 2.1 0.29 7.1 1.1 0.24 4.7 GX 17+2 274.054 -14.005 3.4 16.482 +1.251 20.2 2.68 7.6 0.0 0.00 0.0 4U 1722-30 261.873 -30.825 3.9 356.293 +2.296 2.3 0.36 6.5 1.3 0.29 4.7 1A 1743-288 266.683 -28.924 0.0 0.137 -0.201 1.9 0.00 6.7 1.1 0.24 4.5 SLX 1744-299_300 266.876 -29.993 0.0 359.310 -0.899 2.1 0.00 6.7 0.0 0.00 0.0 SLX 1735-269 264.568 -26.996 3.7 0.793 +2.401 2.5 0.37 7.0 0.0 0.00 0.0 GX 13+1 273.623 -17.137 4.9 13.531 +0.123 4.2 0.84 5.0 0.0 0.00 0.0 Swift J174535.5-2901 266.307 -29.007 0.0 359.895 +0.037 1.5 0.00 5.4 0.0 0.00 0.0 OAO 1657-415 255.239 -41.648 5.1 344.392 +0.303 8.2 1.70 4.8 0.0 0.00 0.0 3A 1728-169 262.953 -16.974 0.0 8.512 +9.016 2.8 0.00 4.0 0.0 0.00 0.0 H 1705-440 257.248 -44.202 6.2 343.249 -2.414 16.0 0.00 3.9 0.0 0.00 0.0 IGR J17488-3253 267.211 -32.950 5.4 356.922 -2.669 1.4 0.31 4.5 0.0 0.00 0.0 GRS 1734-292 264.287 -29.195 6.3 358.801 +1.434 1.1 0.29 3.8 0.0 0.00 0.0 IGR J17391-3021 264.819 -30.321 5.8 358.097 +0.442 1.4 0.33 4.2 0.0 0.00 0.0 GRO J1744-28 266.026 -28.677 6.5 0.047 +0.419 1.0 0.00 3.7 0.0 0.00 0.0 NEW SOURCE 266.313 -25.556 4.1 2.843 +1.832 1.8 0.29 6.1 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 1742-294 266.542 -29.526 359.559 -0.409 1.3 0.26 5.2 0.8 0.16 5.0 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.27 3.3 0.3 0.16 1.7 4U 1722-30 261.888 -30.802 356.320 +2.298 2.5 0.48 5.2 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 3.6 1.02 3.5 1.2 0.54 2.2 GX 1+4 263.009 -24.746 1.937 +4.795 1.5 0.92 1.6 1.9 0.61 3.1 GX 3+1 266.983 -26.567 2.290 +0.792 30.6 0.42 72.4 3.5 0.22 16.0 GX 354-0 262.990 -33.833 354.304 -0.150 19.2 1.09 17.7 3.8 0.83 4.6 GX 5-1 270.280 -25.074 5.080 -1.013 99.5 1.80 55.3 17.9 0.87 20.5 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.3 0.26 5.0 0.3 0.17 1.7 XTE J1739-285 264.975 -28.496 359.714 +1.298 1.6 0.26 6.2 0.4 0.16 2.3 NEW SOURCE 265.603 -25.007 2.975 +2.665 2.6 0.63 4.1 0.4 0.36 1.1 1A 1743-288 266.757 -28.893 0.197 -0.241 1.1 0.27 4.1 0.2 0.17 1.4 NEW SOURCE 265.979 -22.396 5.384 +3.739 10.3 2.62 3.9 0.0 0.00 0.0