INTEGRAL Galactic Bulge Monitoring Revolution 0841: Observation start 2009-09-03T04:09 = MJD 55077.173
Total Observation GTI = 16485 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 1+4 263.006 -24.748 0.8 1.933 +4.796 14.7 0.34 43.4 0.0 0.00 0.0 1E 1740.7-2942 265.988 -29.748 0.8 359.117 -0.114 12.2 0.28 43.7 7.7 0.24 31.8 GX 5-1 270.284 -25.080 0.8 5.076 -1.019 14.0 0.34 41.1 1.1 0.00 3.9 Ginga 1826-24 277.364 -23.790 1.0 9.277 -6.082 15.9 0.54 29.6 3.4 0.42 8.0 GRS 1758-258 270.296 -25.752 1.1 4.498 -1.361 9.1 0.33 27.6 5.8 0.28 21.1 4U 1700-377 255.977 -37.850 1.1 347.745 +2.176 16.2 0.60 27.0 4.2 0.48 8.8 GX 349+2 256.439 -36.427 1.2 349.102 +2.744 12.4 0.51 24.2 0.0 0.00 0.0 H 1820-303 275.912 -30.369 1.9 2.779 -7.912 5.9 0.40 14.9 0.0 0.00 0.0 4U 1722-30 261.874 -30.802 2.2 356.313 +2.308 3.8 0.31 12.2 1.1 0.25 4.2 3A 1822-371 276.460 -37.116 2.6 356.845 -11.306 5.7 0.56 10.3 0.0 0.00 0.0 SLX 1744-299_300 266.865 -30.016 2.9 359.285 -0.903 2.6 0.29 8.8 1.7 0.25 6.5 GX 17+2 274.025 -14.036 2.8 16.442 +1.261 29.3 3.09 9.5 0.0 0.00 0.0 GX 9+1 270.373 -20.527 4.6 9.073 +1.164 2.5 0.45 5.4 0.0 0.00 0.0 GX 3+1 266.917 -26.587 4.4 2.243 +0.833 1.6 0.29 5.7 0.0 0.00 0.0 SLX 1735-269 264.624 -27.003 4.6 0.813 +2.355 1.5 0.28 5.4 1.0 0.24 3.9 GX 354-0 262.974 -33.830 4.6 354.300 -0.137 1.6 0.30 5.5 0.0 0.00 0.0 MXB 1730-335 263.380 -33.359 4.6 354.879 -0.164 1.6 0.29 5.4 0.0 0.00 0.0 GRS 1734-292 264.431 -29.123 5.5 358.929 +1.367 1.2 0.28 4.5 0.0 0.00 0.0 KS 1741-293 266.176 -29.374 0.0 359.522 -0.058 1.1 0.00 3.9 0.0 0.00 0.0 1E 1742.8-2853 266.483 -28.930 5.7 0.041 -0.055 1.2 0.28 4.3 0.0 0.00 0.0 NEW_1 269.631 -21.361 4.0 8.005 +1.351 2.7 0.42 6.3 4.8 0.73 6.6JEM-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 6.0 1.01 0.6 0.55 MXB 1730-335 263.350 -33.388 354.841 -0.158 8.5 0.75 0.9 0.41 SLX 1735-269 264.571 -26.994 0.796 +2.400 4.2 0.59 1.0 0.44 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.9 0.29 1.5 0.22 1A 1742-294 266.523 -29.515 359.559 -0.389 5.8 0.32 1.1 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 30.5 0.60 4.2 0.35 GX 5-1 270.284 -25.079 5.077 -1.019 101.9 3.10 16.1 1.62
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