INTEGRAL Galactic Bulge Monitoring Revolution 0657: Observation start 2008-02-29T13:05 = MJD 54525.546
Total Observation GTI = 10202 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.296 -26.644 0.4 2.369 +0.512 40.8 0.35 115.2 2.1 0.30 7.1 4U 1700-377 255.983 -37.835 0.8 347.760 +2.182 32.0 0.76 42.2 10.1 0.58 17.3 Ginga 1826-24 277.363 -23.791 1.0 9.276 -6.082 18.1 0.58 31.2 7.3 0.44 16.5 4U 1722-30 261.881 -30.809 1.2 356.311 +2.300 9.4 0.37 25.2 3.0 0.30 10.3 H 1820-303 275.898 -30.365 1.4 2.777 -7.900 10.1 0.50 20.3 0.0 0.00 0.0 GX 3+1 266.971 -26.541 0.0 2.308 +0.814 4.7 0.00 13.3 0.0 0.00 0.0 GRS 1758-258 270.323 -25.704 2.3 4.552 -1.358 4.4 0.38 11.6 2.3 0.30 7.8 GX 9+1 270.374 -20.509 3.2 9.090 +1.172 4.0 0.50 8.0 0.0 0.00 0.0 1E 1740.7-2942 265.976 -29.751 3.5 359.110 -0.107 2.4 0.32 7.4 2.7 0.27 10.1 3A 1822-371 276.485 -37.090 2.7 356.878 -11.313 6.3 0.65 9.8 0.0 0.00 0.0 GX 349+2 256.397 -36.453 3.2 349.061 +2.755 5.1 0.64 8.0 0.0 0.00 0.0 GX 17+2 273.978 -14.070 3.3 16.389 +1.286 25.3 3.24 7.8 0.0 0.00 0.0 GX 354-0 262.971 -33.829 3.3 354.299 -0.134 3.1 0.39 7.8 1.1 0.00 3.6 GX 1+4 262.994 -24.736 3.8 1.937 +4.811 2.9 0.44 6.6 0.0 0.00 0.0 SLX 1735-269 264.525 -26.945 4.3 0.815 +2.461 2.1 0.36 5.9 0.0 0.00 0.0 1A 1742-294 266.476 -29.563 4.3 359.497 -0.379 1.9 0.32 5.8 0.0 0.00 0.0 IGR J17252-3616 261.239 -36.307 4.2 351.450 -0.329 2.9 0.48 6.0 0.0 0.00 0.0 GX 5-1 270.329 -25.120 4.4 5.062 -1.074 2.1 0.38 5.6 0.0 0.00 0.0 MXB 1730-335 263.233 -33.385 0.0 354.790 -0.075 2.0 0.00 5.0 0.0 0.00 0.0 1E 1742.8-2853 266.545 -28.931 6.3 0.068 -0.102 1.2 0.32 3.9 1.0 0.00 3.7 SLX 1744-299_300 266.803 -30.048 6.8 359.230 -0.874 1.1 0.32 3.5 0.0 0.00 0.0 IGR J16558-4150 253.934 -41.753 0.0 343.705 +1.002 7.3 0.00 3.8 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== MXB 1730-335 263.350 -33.388 354.841 -0.158 7.7 1.29 0.8 0.79 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.2 0.36 0.6 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 29.3 0.68 3.9 0.36 GX 5-1 270.284 -25.079 5.077 -1.019 63.3 2.32 4.1 1.06 GRO J1750-27 267.300 -26.647 2.368 +0.508 12.5 0.63 9.5 0.40
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