INTEGRAL Galactic bulge Monitoring
Revolution 0359: Observation start 2005-09-23T00:41 = MJD 53636.029
Total Observation GTI = 12254 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 5-1 270.286 -25.076 0.6 5.081 -1.018 21.9 0.36 60.5 0.0 0.00 0.0 4U 1700-377 255.985 -37.846 0.7 347.752 +2.173 31.4 0.65 48.4 10.8 0.49 22.2 GRS 1758-258 270.304 -25.732 0.9 4.519 -1.358 12.3 0.32 37.9 8.0 0.26 31.2 GX 354-0 262.992 -33.841 0.8 354.298 -0.156 13.7 0.36 38.5 3.0 0.28 10.7 Ginga 1826-24 277.348 -23.792 1.0 9.269 -6.070 18.0 0.57 31.7 6.5 0.43 14.9 GX 349+2 256.443 -36.419 1.1 349.110 +2.746 16.4 0.58 28.1 0.0 0.00 0.0 1E 1740.7-2942 265.963 -29.744 1.1 359.110 -0.094 8.5 0.30 28.0 5.0 0.25 20.0 GX 1+4 263.012 -24.734 1.1 1.948 +4.799 10.2 0.37 27.5 0.0 0.00 0.0 H 1820-303 275.913 -30.333 2.2 2.811 -7.896 5.7 0.46 12.6 0.0 0.00 0.0 GRO J1655-40 253.477 -39.815 2.4 344.994 +2.489 13.1 1.20 10.9 10.0 0.91 11.0 GX 9+1 270.369 -20.530 2.8 9.069 +1.166 4.1 0.43 9.5 0.0 0.00 0.0 3A 1822-371 276.482 -37.084 3.4 356.883 -11.308 4.5 0.59 7.6 0.0 0.00 0.0 IGR J17464-3213 266.592 -32.239 2.8 357.263 -1.855 2.9 0.31 9.5 2.1 0.25 8.5 KS 1741-293 266.210 -29.337 0.0 359.569 -0.064 2.2 0.00 7.7 0.0 0.00 0.0 SLX 1735-269 264.575 -27.013 3.5 0.782 +2.387 2.4 0.33 7.2 1.7 0.27 6.4 XTE J1739-285 265.054 -28.420 3.8 359.816 +1.280 2.0 0.30 6.7 0.0 0.00 0.0 GX 3+1 267.053 -26.578 3.5 2.313 +0.733 2.2 0.30 7.4 0.0 0.00 0.0 SLX 1744-299_300 266.883 -30.013 4.9 359.296 -0.915 1.7 0.33 5.1 0.0 0.00 0.0 GX 17+2 274.037 -14.034 4.1 16.449 +1.252 14.9 2.44 6.1 0.0 0.00 0.0 GX 13+1 273.508 -17.149 5.6 13.467 +0.214 3.8 0.86 4.4 0.0 0.00 0.0 IGR J17541-2252 268.620 -22.925 5.2 6.181 +1.376 1.7 0.00 4.7 0.0 0.00 0.0 IGR J17456-2901 266.399 -29.008 0.0 359.936 -0.033 1.3 0.00 4.6 0.0 0.00 0.0 GRS 1734-292 264.387 -29.130 4.7 358.903 +1.396 1.6 0.30 5.3 0.0 0.00 0.0 IGR J18027-2016 270.641 -20.219 0.0 9.465 +1.098 2.0 0.00 4.2 0.0 0.00 0.0 Oph Cluster 258.061 -23.289 6.2 0.611 +9.357 1.8 0.00 3.9 0.0 0.00 0.0 IGR J17252-3616 261.390 -36.284 5.6 351.538 -0.416 1.9 0.43 4.4 0.0 0.00 0.0 V2400 Oph 258.169 -24.187 6.6 359.924 +8.761 1.6 0.00 3.6 0.0 0.00 0.0 IGR J18048-1455 271.192 -14.960 5.8 14.309 +3.220 6.3 1.48 4.2 0.0 0.00 0.0 GRS 1747-312 267.746 -31.304 6.9 358.570 -2.215 1.1 0.00 3.5 0.0 0.00 0.0 1A 1742-294 266.588 -29.502 0.0 359.600 -0.431 1.0 0.00 3.4 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 1742-294 266.527 -29.521 359.556 -0.396 6.1 0.26 23.8 1.2 0.15 7.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.5 0.25 6.0 1.1 0.15 7.1 4U 1722-30 261.888 -30.802 356.320 +2.298 6.4 0.58 11.1 1.4 0.40 3.6 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.2 0.30 7.3 0.3 0.19 1.8 GX 3+1 266.986 -26.570 2.289 +0.788 25.6 0.39 65.4 2.7 0.20 13.5 GX 354-0 262.989 -33.835 354.302 -0.150 13.7 1.17 11.7 4.6 0.86 5.3 GX 5-1 270.288 -25.077 5.080 -1.020 95.2 1.50 63.6 18.0 0.74 24.2 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.2 0.33 3.6 0.3 0.20 1.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.2 0.26 4.8 0.4 0.15 2.3 XTE J1739-285 264.975 -28.496 359.714 +1.298 0.8 0.27 3.1 0.4 0.16 2.7 NEW SOURCE 271.996 -28.275 3.035 -3.915 4.1 0.80 5.1 0.0 0.00 0.0 NEW SOURCE 272.577 -28.855 2.770 -4.641 4.5 0.90 4.9 0.0 0.00 0.0 NEW SOURCE 270.390 -24.958 5.230 -1.042 4.9 1.37 3.6 1.2 0.71 1.7 NEW SOURCE 271.162 -27.508 3.348 -2.899 2.5 0.61 4.1 0.0 0.00 0.0