INTEGRAL Galactic Bulge Monitoring Revolution 0840: Observation start 2009-08-31T03:43 = MJD 55074.156
Total Observation GTI = 13532 seconds
ISGRI
ISGRI significance mosaic images. Left: ISGRI 18-40 keV. Right: 40-100 keVSources 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
OSA7
, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 206 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 103 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 andNEW
sources < 6σ towards the border of the image may be spurious.
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 1700-377 255.987 -37.845 0.6 347.754 +2.172 39.9 0.61 65.6 11.5 0.48 23.7 GX 1+4 263.009 -24.747 0.7 1.936 +4.794 16.8 0.36 46.5 0.0 0.00 0.0 1E 1740.7-2942 265.981 -29.746 0.8 359.117 -0.108 12.1 0.28 42.6 7.6 0.25 31.0 GX 5-1 270.284 -25.080 0.8 5.076 -1.019 14.8 0.38 38.5 0.0 0.00 0.0 GRS 1758-258 270.303 -25.747 1.1 4.505 -1.364 9.7 0.36 26.7 5.9 0.30 19.4 Ginga 1826-24 277.374 -23.807 1.3 9.266 -6.098 13.2 0.59 22.3 4.4 0.47 9.5 GX 349+2 256.448 -36.442 2.4 349.094 +2.729 6.0 0.53 11.4 0.0 0.00 0.0 H 1820-303 275.935 -30.396 2.3 2.763 -7.942 5.2 0.45 11.7 0.0 0.00 0.0 4U 1722-30 261.901 -30.796 2.8 356.331 +2.292 3.0 0.31 9.5 1.6 0.26 6.0 3A 1822-371 276.420 -37.130 2.8 356.819 -11.283 5.1 0.55 9.3 0.0 0.00 0.0 SLX 1744-299_300 266.865 -30.048 2.8 359.257 -0.920 2.5 0.27 9.4 1.0 0.00 4.4 OAO 1657-415 255.193 -41.675 3.4 344.350 +0.314 8.1 1.07 7.6 0.0 0.00 0.0 GX 9+1 270.417 -20.536 3.4 9.085 +1.124 3.6 0.48 7.5 0.0 0.00 0.0 IGR J17252-3616 261.311 -36.234 4.3 351.544 -0.336 2.4 0.41 5.8 0.0 0.00 0.0 Oph Cluster 258.042 -23.334 5.7 0.564 +9.346 1.9 0.46 4.3 0.0 0.00 0.0 GX 3+1 266.993 -26.545 4.5 2.314 +0.796 1.7 0.30 5.6 0.0 0.00 0.0 GX 354-0 262.950 -33.841 4.5 354.279 -0.127 1.7 0.31 5.5 0.0 0.00 0.0 MXB 1730-335 263.305 -33.392 4.4 354.817 -0.129 1.8 0.31 5.7 0.0 0.00 0.0 GRS 1734-292 264.281 -29.133 4.9 358.851 +1.472 1.5 0.30 5.0 0.0 0.00 0.0 IGR J17354-3255 263.760 -32.972 6.1 355.377 -0.221 1.3 0.32 4.0 0.0 0.00 0.0 XB 1832-330 278.920 -32.977 6.5 1.540 -11.355 2.1 0.00 3.8 0.0 0.00 0.0 1A 1742-294 266.552 -29.542 5.6 359.550 -0.425 1.2 0.27 4.4 0.0 0.00 0.0 GX 17+2 274.049 -14.052 0.0 16.439 +1.233 11.9 0.00 3.6 0.0 0.00 0.0 NEW_1 269.689 -21.370 5.1 8.024 +1.300 2.2 0.45 4.8 0.0 0.00 0.0JEM-X
JEM-X significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.Note: Sources labelled were detected in the 3-10 keV image > 5σ and 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 ~ 88 cps); B = 10-25 keV (1 Crab ~ 32 cps).NOTE: 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.
JEM-X Detected Sources in 3-10 keV (A) and 10-25 keV (B).Source Name RA dec l b A(cps) +/- B(cps) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 5.6 0.84 0.9 0.58 MXB 1730-335 263.350 -33.388 354.841 -0.158 14.9 0.68 2.4 0.47 1A 1742-294 266.523 -29.515 359.559 -0.389 5.7 0.33 1.1 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 29.8 0.66 3.1 0.36 GX 5-1 270.284 -25.079 5.077 -1.019 91.4 2.71 14.9 1.36
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