INTEGRAL Galactic Bulge Monitoring Revolution 0776: Observation start 2009-02-21T09:55 = MJD 54883.414
Total Observation GTI = 12202 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 354-0 262.988 -33.832 0.7 354.304 -0.147 18.3 0.35 52.0 4.5 0.30 15.2 4U 1700-377 255.989 -37.843 0.7 347.757 +2.172 37.4 0.78 47.7 7.8 0.62 12.6 1E 1740.7-2942 265.979 -29.744 0.9 359.117 -0.105 12.0 0.31 38.3 8.1 0.27 29.7 Ginga 1826-24 277.370 -23.801 1.0 9.270 -6.092 16.1 0.54 30.0 5.6 0.43 12.8 GX 5-1 270.283 -25.069 1.3 5.085 -1.012 7.8 0.34 22.9 0.0 0.00 0.0 H 1820-303 275.931 -30.350 1.6 2.803 -7.918 7.9 0.46 17.2 0.0 0.00 0.0 GX 1+4 263.024 -24.732 1.9 1.956 +4.790 5.0 0.34 14.8 0.0 0.00 0.0 GRS 1758-258 270.325 -25.714 2.1 4.544 -1.364 4.5 0.34 13.2 3.2 0.29 11.3 OAO 1657-415 255.215 -41.649 2.4 344.380 +0.317 17.2 1.52 11.3 0.0 0.00 0.0 3A 1822-371 276.441 -37.110 2.7 356.845 -11.290 6.4 0.64 9.9 0.0 0.00 0.0 SLX 1735-269 264.604 -26.988 3.1 0.817 +2.379 2.8 0.34 8.2 0.0 0.00 0.0 4U 1722-30 261.924 -30.834 3.2 356.310 +2.255 2.8 0.34 8.2 0.0 0.00 0.0 GX 349+2 256.398 -36.426 2.9 349.084 +2.771 5.4 0.60 9.0 0.0 0.00 0.0 GX 3+1 266.969 -26.568 2.8 2.283 +0.802 3.0 0.32 9.2 0.0 0.00 0.0 SLX 1744-299_300 266.865 -30.013 3.0 359.288 -0.901 2.9 0.32 8.8 0.0 0.00 0.0 IGR J18027-2016 270.696 -20.292 3.4 9.427 +1.016 3.4 0.00 7.7 0.0 0.00 0.0 GX 9+1 270.357 -20.541 0.0 9.054 +1.170 3.1 0.00 7.1 0.0 0.00 0.0 MXB 1730-335 263.326 -33.372 0.0 354.843 -0.132 2.1 0.00 6.0 0.0 0.00 0.0 IGR J17252-3616 261.251 -36.314 5.4 351.450 -0.341 2.1 0.45 4.5 0.0 0.00 0.0 SAX J1750.8-2900 267.618 -28.995 0.0 0.497 -0.939 1.5 0.00 5.3 0.0 0.00 0.0 GX 17+2 274.017 -13.996 4.8 16.473 +1.287 8.1 1.57 5.2 0.0 0.00 0.0 IGR J17536-2339 268.341 -23.576 6.5 5.490 +1.267 1.2 0.33 3.7 0.0 0.00 0.0 GRS 1741.9-2853 266.314 -28.979 5.7 359.922 +0.046 1.3 0.29 4.3 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 3.2 0.41 0.9 0.26 GX 3+1 266.983 -26.564 2.294 +0.794 34.7 0.56 5.3 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 101.3 1.66 10.7 0.71
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