INTEGRAL Galactic bulge Monitoring
Revolution 0670: Observation start 2008-04-08T10:17 = MJD 54564.429
Total Observation GTI = 22388 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17473-2721 266.827 -27.341 0.5 1.556 +0.511 22.8 0.26 88.7 11.6 0.20 57.2 GRO J1750-27 267.287 -26.642 0.6 2.366 +0.520 17.2 0.30 58.0 0.0 0.00 0.0 4U 1700-377 255.999 -37.859 0.8 347.749 +2.157 22.2 0.52 42.2 6.6 0.39 16.7 GX 5-1 270.274 -25.082 0.8 5.070 -1.012 12.6 0.30 42.0 0.0 0.00 0.0 H 1820-303 275.913 -30.366 0.8 2.781 -7.911 16.4 0.41 39.7 0.0 0.00 0.0 Ginga 1826-24 277.360 -23.788 0.9 9.278 -6.078 19.1 0.52 36.8 7.9 0.38 20.8 4U 1722-30 261.888 -30.797 0.9 356.324 +2.302 9.0 0.27 33.5 3.7 0.21 17.6 GRS 1758-258 270.303 -25.738 1.4 4.513 -1.359 6.1 0.29 21.0 3.9 0.22 17.3 GX 349+2 256.461 -36.412 1.4 349.124 +2.739 9.4 0.46 20.6 0.0 0.00 0.0 XTE J1810-189 272.582 -19.052 1.4 11.375 +0.072 10.0 0.50 20.0 3.7 0.37 9.9 SAX J1750.8-2900 267.580 -29.053 1.6 0.431 -0.940 4.9 0.27 18.0 2.5 0.21 12.1 1E 1740.7-2942 265.964 -29.753 1.7 359.103 -0.099 4.1 0.25 16.4 2.6 0.20 13.1 GX 354-0 262.985 -33.845 1.6 354.292 -0.153 4.7 0.27 17.3 0.0 0.00 0.0 GX 9+1 270.380 -20.532 2.1 9.072 +1.156 5.1 0.41 12.7 0.0 0.00 0.0 GX 3+1 266.886 -26.601 2.4 2.217 +0.849 3.3 0.00 11.3 0.0 0.00 0.0 3A 1822-371 276.476 -37.099 2.3 356.866 -11.310 6.6 0.56 11.7 0.0 0.00 0.0 IGR J17391-3021 264.796 -30.320 2.6 358.087 +0.459 2.9 0.28 10.3 0.0 0.00 0.0 SLX 1735-269 264.579 -27.036 3.8 0.764 +2.372 1.6 0.25 6.6 1.3 0.19 6.6 3A 1728-169 262.956 -16.992 3.4 8.498 +9.004 5.0 0.66 7.6 0.0 0.00 0.0 IGR J18027-2016 270.732 -20.272 0.0 9.461 +0.997 2.8 0.00 7.0 0.0 0.00 0.0 SLX 1744-299_300 266.812 -29.957 3.8 359.311 -0.833 1.7 0.25 6.6 0.9 0.20 4.6 XTE J1709-267 257.332 -26.668 4.7 357.439 +7.936 1.9 0.36 5.3 0.0 0.00 0.0 SAX J1810.8-2609 272.663 -26.087 5.3 5.243 -3.383 1.5 0.32 4.6 0.0 0.00 0.0 SLX 1737-282 265.177 -28.299 7.5 359.975 +1.252 0.9 0.27 3.2 0.0 0.00 0.0 GX 1+4 262.994 -24.792 5.5 1.890 +4.781 1.4 0.31 4.5 0.0 0.00 0.0 1A 1743-288 266.734 -28.882 7.5 0.196 -0.218 0.8 0.27 3.2 0.0 0.00 0.0 Swift J171707.3-3640 259.366 -36.651 6.8 350.310 +0.713 1.4 0.00 3.6 0.0 0.00 0.0 H 1702-429 256.620 -43.021 6.7 343.924 -1.342 6.5 1.79 3.6 0.0 0.00 0.0 MAXI J1836-194 279.035 -19.305 7.0 14.004 -5.435 3.2 0.00 3.5 0.0 0.00 0.0 IGR J17448-3232 266.316 -32.551 6.9 356.875 -1.819 1.0 0.29 3.5 0.0 0.00 0.0 IGR J17200-3116 260.046 -31.260 5.6 355.052 +3.345 1.3 0.30 4.4 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 1742-294 266.541 -29.495 359.585 -0.393 5.2 0.25 20.7 0.7 0.15 4.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.0 0.23 4.4 0.7 0.14 4.6 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.2 0.26 4.7 0.3 0.15 1.7 4U 1722-30 261.888 -30.802 356.320 +2.298 3.9 0.39 10.2 1.9 0.27 7.0 GRO J1750-27 267.300 -26.645 2.370 +0.509 5.1 0.40 12.8 4.6 0.22 20.4 GRS 1734-292 264.367 -29.142 358.883 +1.404 0.8 0.24 3.5 0.2 0.15 1.0 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.7 0.30 5.9 0.3 0.19 1.5 GX 3+1 266.987 -26.559 2.300 +0.793 48.4 0.44 109.8 5.9 0.23 26.1 GX 354-0 262.989 -33.835 354.302 -0.150 15.3 0.73 20.9 3.7 0.55 6.7 GX 5-1 270.280 -25.074 5.080 -1.013 127.0 1.92 66.1 15.7 0.94 16.7 IGR J17391-3021 264.802 -30.339 358.074 +0.445 0.9 0.23 3.9 0.7 0.15 4.7 IGR J17473-2721 266.835 -27.356 1.547 +0.497 6.6 0.32 20.4 3.3 0.19 17.8 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.6 0.31 5.3 0.3 0.18 1.7 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.25 8.2 0.3 0.15 1.7 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.7 0.24 3.1 0.3 0.14 2.4 SAX J1750.8-2900 267.605 -29.032 0.460 -0.948 1.9 0.28 6.6 0.8 0.16 4.9 NEW SOURCE 267.624 -22.818 5.807 +2.221 13.1 2.62 5.0 0.0 0.00 0.0