INTEGRAL Galactic bulge Monitoring
Revolution 0296: Observation start 2005-03-17T18:09 = MJD 53446.757
Total Observation GTI = 12207 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 1700-377 255.986 -37.853 0.6 347.747 +2.168 33.9 0.60 56.2 7.8 0.45 17.2 GX 5-1 270.282 -25.073 0.8 5.082 -1.013 16.3 0.36 44.7 0.0 0.00 0.0 GRS 1758-258 270.296 -25.746 0.8 4.503 -1.358 12.3 0.32 38.5 8.4 0.25 33.3 GX 349+2 256.439 -36.422 0.9 349.106 +2.747 19.6 0.55 35.6 0.0 0.00 0.0 1E 1740.7-2942 265.970 -29.745 0.9 359.112 -0.099 10.1 0.29 34.4 5.9 0.24 24.5 Ginga 1826-24 277.358 -23.796 1.1 9.270 -6.080 16.7 0.61 27.4 5.0 0.46 10.8 GX 354-0 263.014 -33.842 1.2 354.308 -0.171 7.9 0.33 24.2 0.0 0.00 0.0 GRO J1655-40 253.511 -39.841 1.2 344.991 +2.453 29.1 1.14 25.5 11.0 0.83 13.2 4U 1722-30 261.894 -30.794 1.9 356.330 +2.298 4.8 0.33 14.8 2.2 0.26 8.2 IGR J17252-3616 261.308 -36.276 2.1 351.508 -0.357 5.3 0.41 13.0 1.2 0.32 3.7 H 1820-303 275.912 -30.332 2.1 2.812 -7.895 6.1 0.47 12.8 0.0 0.00 0.0 3A 1822-371 276.480 -37.097 2.6 356.870 -11.313 6.1 0.60 10.1 0.0 0.00 0.0 GX 3+1 267.011 -26.591 3.5 2.283 +0.758 2.1 0.29 7.3 0.0 0.00 0.0 GX 9+1 270.364 -20.503 3.3 9.090 +1.183 3.3 0.42 7.8 0.0 0.00 0.0 GX 17+2 274.040 -14.047 3.7 16.438 +1.243 16.5 2.41 6.8 0.0 0.00 0.0 SLX 1735-269 264.585 -27.021 3.7 0.780 +2.376 2.2 0.32 6.9 0.0 0.00 0.0 1A 1742-294 266.519 -29.528 4.2 359.547 -0.393 1.7 0.29 6.0 0.0 0.00 0.0 SLX 1744-299_300 266.801 -29.982 4.6 359.286 -0.838 1.8 0.33 5.4 0.0 0.00 0.0 IGR J17091-3624 257.344 -36.347 5.5 349.603 +2.208 2.3 0.53 4.5 0.0 0.00 0.0 V2400 Oph 258.041 -24.309 5.5 359.755 +8.786 1.9 0.42 4.5 0.0 0.00 0.0 AX J1749.1-2733 267.197 -27.545 7.6 1.551 +0.124 1.1 0.35 3.2 0.0 0.00 0.0 1A 1744-361 267.107 -36.234 5.1 354.054 -4.280 1.9 0.40 4.8 0.0 0.00 0.0 IGR J18027-2016 270.683 -20.239 0.0 9.468 +1.053 1.8 0.00 4.2 0.0 0.00 0.0 3A 1728-169 262.943 -16.953 4.6 8.525 +9.035 3.7 0.69 5.4 0.0 0.00 0.0 GRS 1734-292 264.393 -29.152 5.9 358.887 +1.380 1.2 0.29 4.1 0.0 0.00 0.0 IGR J17475-2822 266.824 -28.335 7.4 0.705 -0.002 1.0 0.29 3.2 0.0 0.00 0.0 SLX 1737-282 265.148 -28.335 7.1 359.932 +1.254 1.0 0.28 3.4 0.0 0.00 0.0 IGR J17473-2721 266.744 -27.391 0.0 1.475 +0.548 1.3 0.00 3.8 0.0 0.00 0.0 GX 13+1 273.570 -17.209 0.0 13.444 +0.133 3.0 0.00 3.7 0.0 0.00 0.0 1A 1743-288 266.659 -28.955 6.5 0.100 -0.200 1.0 0.00 3.7 0.0 0.00 0.0 XTE J1743-363 265.893 -36.400 0.0 353.404 -3.529 1.4 0.00 3.7 0.0 0.00 0.0 XB 1832-330 278.967 -33.028 5.9 1.509 -11.413 2.6 0.64 4.1 2.6 0.48 5.3
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 1742-294 266.528 -29.503 359.572 -0.386 2.5 0.22 11.1 0.6 0.13 4.6 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.0 0.22 9.3 1.2 0.13 9.4 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.23 3.6 0.3 0.13 2.2 4U 1722-30 261.888 -30.802 356.320 +2.298 1.9 0.37 5.2 0.6 0.25 2.4 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.1 0.23 4.8 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 4.511 -1.361 5.1 1.06 4.8 1.2 0.51 2.4 GX 3+1 266.988 -26.562 2.298 +0.791 25.5 0.37 68.8 2.7 0.18 14.9 GX 354-0 262.995 -33.821 354.316 -0.147 12.8 0.85 15.1 3.3 0.59 5.6 GX 5-1 270.283 -25.075 5.080 -1.016 128.3 1.86 68.9 16.9 0.80 21.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.24 4.6 0.3 0.14 2.5 CONFUSED ID 270.243 -25.708 4.512 -1.298 6.6 1.05 6.3 0.9 0.49 1.9 NEW SOURCE 269.824 -27.925 2.401 -2.073 2.6 0.46 5.7 0.4 0.25 1.6 CONFUSED ID 270.383 -25.758 4.532 -1.432 6.7 1.11 6.1 1.4 0.56 2.5 NEW SOURCE 270.089 -28.478 2.036 -2.551 2.6 0.45 5.7 0.0 0.00 0.0 NEW SOURCE 267.827 -24.966 4.055 +0.963 3.2 0.65 4.9 0.0 0.00 0.0 NEW SOURCE 269.494 -24.037 5.623 +0.123 9.1 1.80 5.0 0.0 0.00 0.0