INTEGRAL Galactic Bulge Monitoring Revolution 0836: Observation start 2009-08-20T10:28 = MJD 55063.437
Total Observation GTI = 13161 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+4 263.013 -24.745 0.5 1.939 +4.792 27.2 0.33 83.5 0.0 0.00 0.0 4U 1700-377 255.997 -37.842 0.7 347.761 +2.168 38.1 0.71 53.9 9.3 0.56 16.6 1E 1740.7-2942 265.979 -29.747 0.8 359.115 -0.108 12.0 0.31 38.9 7.7 0.27 28.5 GRS 1758-258 270.316 -25.759 1.0 4.501 -1.380 9.4 0.31 30.1 6.2 0.26 23.5 Ginga 1826-24 277.366 -23.792 1.2 9.276 -6.084 12.4 0.48 25.8 5.0 0.39 12.9 GX 5-1 270.283 -25.074 1.4 5.081 -1.015 6.6 0.31 21.4 0.0 0.00 0.0 H 1820-303 275.923 -30.357 1.6 2.794 -7.915 7.4 0.43 17.2 0.0 0.00 0.0 1A 1742-294 266.537 -29.509 1.8 359.571 -0.396 4.4 0.29 15.2 1.1 0.00 4.2 GX 349+2 256.441 -36.409 1.9 349.118 +2.754 9.8 0.66 14.8 0.0 0.00 0.0 GX 354-0 262.994 -33.813 2.5 354.323 -0.142 3.9 0.36 10.6 0.0 0.00 0.0 4U 1722-30 261.893 -30.810 2.6 356.316 +2.290 3.5 0.34 10.2 1.1 0.29 4.0 GX 17+2 274.029 -14.028 2.7 16.451 +1.262 16.0 1.63 9.8 0.0 0.00 0.0 3A 1822-371 276.420 -37.158 2.7 356.793 -11.296 5.4 0.56 9.6 0.0 0.00 0.0 SLX 1744-299_300 266.841 -30.002 3.4 359.286 -0.878 2.4 0.32 7.6 0.0 0.00 0.0 GX 9+1 270.439 -20.446 4.1 9.174 +1.151 2.6 0.43 6.1 0.0 0.00 0.0 OAO 1657-415 255.222 -41.627 3.7 344.401 +0.326 11.4 1.66 6.9 0.0 0.00 0.0 SLX 1735-269 264.565 -26.990 4.8 0.796 +2.407 1.6 0.31 5.1 0.0 0.00 0.0 1E 1742.8-2853 266.422 -28.875 6.5 0.060 +0.019 1.1 0.29 3.7 0.0 0.00 0.0 GX 3+1 266.940 -26.589 5.1 2.252 +0.814 1.4 0.29 4.8 0.0 0.00 0.0 GRS 1734-292 264.402 -29.115 5.9 358.923 +1.393 1.2 0.29 4.1 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== SLX 1735-269 264.571 -26.994 0.796 +2.400 3.9 0.59 0.9 0.41 1A 1742-294 266.523 -29.515 359.559 -0.389 2.7 0.40 1.2 0.27 GX 3+1 266.983 -26.564 2.294 +0.794 28.1 0.68 3.8 0.38 GX 5-1 270.284 -25.079 5.077 -1.019 112.2 2.16 10.9 0.92 GRO J1750-27 267.303 -26.643 2.373 +0.508 8.5 1.68 0.0 0.00
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