INTEGRAL Galactic bulge Monitoring
Revolution 0291: Observation start 2005-03-02T12:01 = MJD 53431.501
Total Observation GTI = 10981 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 1700-377 255.995 -37.843 0.5 347.759 +2.168 42.5 0.60 70.9 13.5 0.46 29.4 GRS 1758-258 270.304 -25.737 0.8 4.514 -1.360 13.7 0.35 39.6 8.1 0.28 29.2 1E 1740.7-2942 265.987 -29.757 0.9 359.110 -0.118 9.3 0.28 33.5 5.5 0.23 23.7 GX 349+2 256.443 -36.431 0.9 349.101 +2.739 19.4 0.55 35.2 0.0 0.00 0.0 Ginga 1826-24 277.385 -23.777 1.2 9.297 -6.093 15.5 0.62 25.2 5.8 0.48 12.2 GX 1+4 263.012 -24.747 1.4 1.937 +4.792 8.2 0.38 21.6 0.0 0.00 0.0 GX 354-0 262.977 -33.818 1.4 354.311 -0.132 6.4 0.31 20.8 0.0 0.00 0.0 OAO 1657-415 255.223 -41.651 1.6 344.382 +0.311 20.6 1.18 17.5 5.0 0.84 6.0 1A 1742-294 266.464 -29.543 0.0 359.509 -0.360 4.3 0.00 15.4 1.4 0.23 6.3 H 1820-303 275.908 -30.366 2.0 2.780 -7.908 7.2 0.53 13.6 0.0 0.00 0.0 4U 1722-30 261.890 -30.805 2.2 356.318 +2.295 3.7 0.29 12.5 1.8 0.24 7.5 3A 1822-371 276.437 -37.078 2.4 356.872 -11.273 6.6 0.58 11.4 0.0 0.00 0.0 GRO J1655-40 253.478 -39.803 3.1 345.005 +2.496 8.2 0.98 8.3 7.2 0.69 10.3 GX 5-1 270.267 -25.102 3.0 5.050 -1.016 3.1 0.35 8.7 0.0 0.00 0.0 SLX 1735-269 264.560 -26.976 2.7 0.806 +2.419 2.8 0.29 9.6 1.4 0.24 6.1 GX 3+1 266.981 -26.569 3.2 2.288 +0.793 2.5 0.30 8.1 0.0 0.00 0.0 GX 9+1 270.384 -20.545 3.9 9.062 +1.146 3.1 0.49 6.4 0.0 0.00 0.0 GX 17+2 273.971 -13.999 4.1 16.449 +1.325 25.0 4.11 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.908 -29.958 4.7 359.355 -0.905 1.5 0.28 5.3 0.0 0.00 0.0 IGR J17407-2808 265.168 -28.205 4.6 0.051 +1.309 1.5 0.27 5.4 0.0 0.00 0.0 V2400 Oph 258.215 -24.156 4.8 359.974 +8.744 2.2 0.43 5.2 0.0 0.00 0.0 XTE J1710-281 257.531 -28.189 5.2 356.300 +6.903 2.0 0.42 4.7 0.0 0.00 0.0 3A 1728-169 262.913 -16.976 4.7 8.490 +9.048 4.8 0.91 5.2 0.0 0.00 0.0 1E 1742.8-2853 266.456 -28.957 5.7 0.006 -0.049 1.2 0.28 4.3 0.0 0.00 0.0 GRS 1734-292 264.391 -29.121 0.0 358.912 +1.398 1.2 0.00 4.4 0.0 0.00 0.0 XTE J1810-189 272.628 -19.101 5.3 11.353 +0.009 2.6 0.56 4.6 0.0 0.00 0.0 IGR J18027-2016 270.664 -20.186 0.0 9.504 +1.096 2.1 0.00 4.2 0.0 0.00 0.0 XTE J1720-318 260.058 -31.798 6.3 354.614 +3.030 1.3 0.33 3.8 0.0 0.00 0.0 IGR J17252-3616 261.334 -36.166 6.2 351.610 -0.312 1.6 0.00 3.9 0.0 0.00 0.0 IGR J17494-3030 267.329 -30.607 6.2 358.985 -1.551 1.1 0.00 3.9 0.0 0.00 0.0 Oph Cluster 258.051 -23.412 6.9 0.504 +9.294 1.6 0.47 3.5 0.0 0.00 0.0 SGR 1806-20 272.226 -20.458 6.5 9.983 -0.315 1.9 0.00 3.7 0.0 0.00 0.0 SAX J1712.6-3739 258.147 -37.663 6.2 348.921 +0.912 2.2 0.56 3.9 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 1.3 0.22 5.8 0.6 0.13 4.2 1E 1740.7-2942 265.983 -29.740 359.122 -0.106 2.5 0.21 11.9 1.3 0.13 10.1 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.23 3.5 0.0 0.00 0.0 4U 1722-30 261.888 -30.802 356.320 +2.298 1.4 0.32 4.5 0.6 0.21 2.7 GRS 1758-258 270.303 -25.741 4.511 -1.361 4.2 1.12 3.8 1.6 0.53 3.1 GX 3+1 266.980 -26.551 2.302 +0.803 25.7 0.46 55.4 2.5 0.23 11.1 GX 354-0 262.989 -33.835 354.302 -0.150 25.1 0.78 32.0 4.6 0.51 9.0 GX 5-1 270.282 -25.080 5.075 -1.017 99.4 2.01 49.4 5.8 0.80 7.3 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.4 0.23 10.3 0.4 0.13 3.1 NEW SOURCE 271.381 -25.659 5.059 -2.166 9.9 1.86 5.3 0.0 0.00 0.0 NEW SOURCE 269.277 -23.891 5.650 +0.368 9.6 2.22 4.3 0.0 0.00 0.0 NEW SOURCE 271.917 -27.789 3.428 -3.619 5.0 0.98 5.1 0.9 0.53 1.8 NEW SOURCE 270.099 -25.548 4.587 -1.106 5.1 1.08 4.7 0.0 0.00 0.0 NEW SOURCE 266.279 -25.290 3.054 +1.996 2.5 0.80 3.1 1.2 0.43 2.7