INTEGRAL Galactic Bulge Monitoring Revolution 0785: Observation start 2009-03-19T06:43 = MJD 54909.281
Total Observation GTI = 12032 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 1700-377 255.990 -37.842 0.5 347.757 +2.172 46.1 0.57 80.9 11.6 0.47 24.7 1E 1740.7-2942 265.975 -29.750 0.8 359.110 -0.106 12.7 0.29 44.3 7.4 0.26 29.0 GX 5-1 270.284 -25.078 1.1 5.078 -1.018 9.5 0.35 27.2 0.0 0.00 0.0 GX 1+4 263.024 -24.748 1.3 1.942 +4.782 7.3 0.33 21.9 0.0 0.00 0.0 1A 1742-294 266.511 -29.513 1.3 359.556 -0.380 6.7 0.30 22.0 2.7 0.00 10.2 Ginga 1826-24 277.364 -23.803 1.3 9.265 -6.088 15.3 0.68 22.4 6.6 0.55 12.1 GRS 1758-258 270.298 -25.743 1.4 4.507 -1.358 7.5 0.37 20.1 5.5 0.32 17.4 GX 349+2 256.404 -36.418 1.7 349.092 +2.772 9.1 0.53 17.1 0.0 0.00 0.0 H 1820-303 275.922 -30.357 1.7 2.794 -7.914 7.7 0.47 16.1 0.0 0.00 0.0 XTE J1709-267 257.407 -26.622 3.1 357.516 +7.909 3.4 0.40 8.5 0.0 0.00 0.0 3A 1822-371 276.439 -37.069 2.9 356.881 -11.271 5.7 0.63 9.0 0.0 0.00 0.0 4U 1722-30 261.885 -30.780 2.9 356.337 +2.312 3.2 0.36 9.0 1.3 0.30 4.1 GX 9+1 270.344 -20.570 2.9 9.022 +1.166 4.2 0.46 9.1 0.0 0.00 0.0 GX 3+1 266.973 -26.581 4.7 2.274 +0.793 1.8 0.35 5.3 0.0 0.00 0.0 IGR J17252-3616 261.325 -36.280 4.7 351.512 -0.371 2.0 0.38 5.3 0.0 0.00 0.0 SLX 1735-269 264.575 -27.041 4.0 0.758 +2.372 2.0 0.31 6.4 1.2 0.28 4.3 GX 354-0 262.947 -33.814 4.0 354.301 -0.109 2.2 0.35 6.3 0.0 0.00 0.0 V2400 Oph 258.079 -24.265 0.0 359.812 +8.783 1.7 0.00 4.0 0.0 0.00 0.0 1H 1746-370 267.489 -37.063 5.8 353.495 -4.967 1.5 0.37 4.2 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 10.4 0.79 2.0 0.52 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.34 1.6 0.24 1A 1742-294 266.523 -29.515 359.559 -0.389 2.1 0.34 1.0 0.23 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.34 0.4 0.25 GX 3+1 266.983 -26.564 2.294 +0.794 35.0 0.76 3.3 0.40 GX 5-1 270.284 -25.079 5.077 -1.019 90.3 4.87 7.6 1.96
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