INTEGRAL Galactic bulge Monitoring
Revolution 0661: Observation start 2008-03-12T18:32 = MJD 54537.773
Total Observation GTI = 12235 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.296 -26.646 0.4 2.368 +0.512 33.6 0.34 98.9 1.5 0.27 5.5 4U 1700-377 255.987 -37.844 0.5 347.754 +2.173 58.2 0.76 76.9 16.5 0.57 28.7 Ginga 1826-24 277.360 -23.797 1.2 9.269 -6.082 17.5 0.73 23.9 7.2 0.55 12.9 4U 1722-30 261.890 -30.809 1.2 356.315 +2.293 8.8 0.36 24.2 3.0 0.29 10.2 H 1820-303 275.888 -30.353 1.8 2.784 -7.886 11.2 0.71 15.8 0.0 0.00 0.0 GX 3+1 266.963 -26.579 0.0 2.271 +0.801 5.0 0.00 14.4 0.0 0.00 0.0 GX 5-1 270.302 -25.078 2.2 5.086 -1.032 5.3 0.42 12.6 0.0 0.00 0.0 GRS 1758-258 270.294 -25.748 2.1 4.500 -1.358 4.8 0.38 12.7 3.2 0.30 10.6 1E 1740.7-2942 265.994 -29.760 2.5 359.111 -0.125 4.0 0.37 10.7 1.7 0.31 5.5 GX 349+2 256.437 -36.435 2.4 349.095 +2.740 6.8 0.62 11.1 0.0 0.00 0.0 OAO 1657-415 255.208 -41.670 2.7 344.360 +0.308 14.9 1.56 9.6 0.0 0.00 0.0 3A 1822-371 276.429 -37.149 2.9 356.804 -11.298 7.3 0.82 8.9 0.0 0.00 0.0 GX 9+1 270.491 -20.529 4.2 9.126 +1.067 3.3 0.55 6.0 0.0 0.00 0.0 SLX 1735-269 264.597 -26.971 4.2 0.828 +2.393 2.0 0.34 5.9 0.0 0.00 0.0 GX 1+4 263.003 -24.756 4.4 1.926 +4.794 2.3 0.40 5.7 0.0 0.00 0.0 XTE J1810-189 272.621 -19.067 4.4 11.380 +0.032 3.9 0.70 5.6 0.0 0.00 0.0 GX 354-0 262.963 -33.869 4.4 354.262 -0.151 2.1 0.37 5.6 0.0 0.00 0.0 3A 1728-169 262.985 -16.888 4.8 8.602 +9.035 4.2 0.82 5.1 0.0 0.00 0.0 IGR J17456-2901 266.414 -28.933 5.3 0.006 -0.005 1.5 0.33 4.6 0.0 0.00 0.0 SLX 1744-299_300 266.897 -30.047 5.2 359.273 -0.942 1.9 0.39 4.8 0.0 0.00 0.0 IGR J17200-3116 260.014 -31.247 4.7 355.047 +3.376 1.9 0.36 5.3 0.0 0.00 0.0 4U 1735-444 264.785 -44.541 5.2 345.992 -7.067 20.1 4.26 4.7 0.0 0.00 0.0 IGR J17586-2129 269.721 -21.388 5.8 8.023 +1.265 2.0 0.47 4.2 0.0 0.00 0.0 GX 17+2 273.996 -14.045 4.8 16.420 +1.282 17.9 3.46 5.2 0.0 0.00 0.0 Swift J1753.7-2544 268.318 -25.703 7.1 3.646 +0.205 1.2 0.35 3.4 0.0 0.00 0.0 XTE J1709-267 257.434 -26.554 6.1 357.586 +7.929 1.8 0.00 4.0 0.0 0.00 0.0 IGR J17464-3213 266.473 -32.287 6.0 357.169 -1.794 1.5 0.37 4.1 0.0 0.00 0.0 GRS 1734-292 264.393 -29.230 6.1 358.821 +1.337 1.2 0.31 4.0 0.0 0.00 0.0 SAX J1750.8-2900 267.479 -29.037 6.5 0.399 -0.856 1.2 0.00 3.7 0.0 0.00 0.0 Swift J175759.9-2246 269.563 -22.797 7.0 6.729 +0.689 1.5 0.44 3.5 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 -29.504 359.568 -0.383 5.2 0.32 16.2 1.2 0.21 5.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.2 0.30 3.9 0.6 0.20 3.1 4U 1722-30 261.888 -30.802 356.320 +2.298 4.5 0.36 12.5 1.7 0.28 6.2 GRO J1750-27 267.298 -26.650 2.365 +0.508 13.8 0.53 26.0 9.7 0.34 28.8 GRS 1734-292 264.367 -29.142 358.883 +1.404 0.8 0.27 3.1 0.4 0.18 2.1 GX 3+1 266.983 -26.559 2.297 +0.796 52.1 0.55 94.2 6.7 0.31 21.8 GX 354-0 262.997 -33.832 354.308 -0.154 10.7 0.82 13.0 2.2 0.65 3.4 GX 5-1 270.287 -25.081 5.077 -1.022 120.0 3.83 31.3 11.1 1.97 5.6 MXB 1730-335 263.350 -33.388 354.841 -0.158 4.4 0.60 7.3 0.0 0.00 0.0 NEW SOURCE 271.045 -26.572 4.115 -2.350 12.3 2.68 4.6 1.6 1.48 1.1 NEW SOURCE 265.507 -23.267 4.412 +3.654 6.2 1.46 4.3 0.0 0.00 0.0 NEW SOURCE 269.845 -25.333 4.659 -0.800 8.8 2.05 4.3 0.0 0.00 0.0 NEW SOURCE 270.515 -25.051 5.205 -1.186 14.2 3.87 3.7 0.0 0.00 0.0