INTEGRAL Galactic Bulge Monitoring Revolution 0856: Observation start 2009-10-16T19:49 = MJD 55120.827
Total Observation GTI = 12525 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 1700-377 255.991 -37.843 0.4 347.757 +2.171 96.8 0.75 128.5 20.7 0.59 35.2 GX 1+4 263.009 -24.746 0.7 1.937 +4.795 18.1 0.35 52.5 0.0 0.00 0.0 1E 1740.7-2942 265.978 -29.744 0.9 359.117 -0.105 12.1 0.33 36.4 7.6 0.29 26.4 GRS 1758-258 270.293 -25.744 1.3 4.503 -1.354 7.8 0.35 22.2 4.9 0.30 16.6 Ginga 1826-24 277.375 -23.792 1.4 9.280 -6.092 12.5 0.59 21.2 4.7 0.48 9.9 IGR J17586-2129 269.657 -21.372 1.9 8.007 +1.324 6.2 0.42 14.6 0.0 0.00 0.0 4U 1722-30 261.866 -30.836 2.7 356.281 +2.295 3.2 0.33 9.7 1.5 0.27 5.5 H 1820-303 275.929 -30.368 2.7 2.786 -7.924 4.7 0.47 9.9 0.0 0.00 0.0 GX 349+2 256.406 -36.434 3.0 349.081 +2.760 5.3 0.61 8.7 0.0 0.00 0.0 GX 5-1 270.319 -25.069 3.0 5.101 -1.041 3.1 0.35 8.8 0.0 0.00 0.0 3A 1822-371 276.458 -37.100 3.3 356.860 -11.298 5.0 0.63 7.8 0.0 0.00 0.0 GX 9+1 270.353 -20.517 4.7 9.073 +1.185 2.6 0.50 5.2 0.0 0.00 0.0 GX 3+1 266.990 -26.549 4.6 2.309 +0.796 1.8 0.32 5.5 0.0 0.00 0.0 SLX 1744-299_300 266.809 -29.963 5.0 359.305 -0.834 1.6 0.31 5.0 1.5 0.27 5.3 XB 1832-330 278.934 -32.999 5.0 1.524 -11.376 2.9 0.59 4.9 0.0 0.00 0.0 IGR J17354-3255 263.814 -32.928 4.9 355.438 -0.235 1.7 0.34 5.0 0.0 0.00 0.0 SLX 1735-269 264.627 -26.981 5.3 0.834 +2.365 1.7 0.36 4.7 0.0 0.00 0.0 3A 1728-169 262.863 -16.971 6.5 8.468 +9.090 2.6 0.70 3.7 0.0 0.00 0.0 GRS 1734-292 264.352 -29.158 5.3 358.863 +1.406 1.6 0.33 4.7 0.0 0.00 0.0 1E 1742.9-2849 266.566 -28.886 5.8 0.116 -0.094 1.3 0.31 4.2 0.0 0.00 0.0 GX 17+2 273.948 -14.013 6.0 16.426 +1.338 11.9 2.95 4.0 0.0 0.00 0.0 IGR J17331-2406 263.346 -24.214 0.0 2.552 +4.825 1.5 0.00 3.7 0.0 0.00 0.0 NEW_1 254.904 -12.597 3.9 7.891 +17.922 38.0 5.65 6.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.37 0.0 0.00 1A 1742-294 266.523 -29.515 359.559 -0.389 3.8 0.36 0.0 0.00 GX 3+1 266.983 -26.564 2.294 +0.794 14.1 0.54 0.0 0.00 GX 5-1 270.284 -25.079 5.077 -1.019 18.9 1.50 0.0 0.00
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