INTEGRAL Galactic Bulge Monitoring Revolution 0491: Observation start 2006-10-20 = MJD 54028
Total Observation GTI = 12228 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 5-1 270.284 -25.077 0.5 5.079 -1.018 25.6 0.32 80.4 1.0 0.00 3.8 GX 1+4 263.007 -24.746 0.6 1.936 +4.796 21.2 0.31 67.3 0.0 0.00 0.0 4U 1700-377 255.998 -37.848 1.0 347.757 +2.164 18.4 0.62 29.8 5.7 0.47 12.1 Ginga 1826-24 277.375 -23.794 1.1 9.278 -6.092 16.6 0.58 28.6 5.2 0.44 11.8 GX 349+2 256.433 -36.419 1.2 349.106 +2.752 14.6 0.57 25.6 0.0 0.00 0.0 GRS 1758-258 270.311 -25.747 1.2 4.508 -1.370 8.0 0.33 24.3 6.0 0.26 22.7 1E 1740.7-2942 265.978 -29.746 1.2 359.115 -0.106 7.2 0.29 25.3 4.3 0.24 18.1 H 1820-303 275.906 -30.363 1.3 2.782 -7.904 10.2 0.45 22.9 0.0 0.00 0.0 IGR J17497-2821 267.405 -28.363 1.4 0.944 -0.454 6.5 0.31 21.1 4.0 0.26 15.6 GX 354-0 262.990 -33.835 1.7 354.302 -0.151 5.3 0.32 16.4 0.0 0.00 0.0 4U 1722-30 261.885 -30.792 2.5 356.326 +2.306 3.4 0.32 10.6 1.5 0.25 5.9 3A 1822-371 276.469 -37.102 2.5 356.861 -11.307 6.7 0.62 10.9 0.0 0.00 0.0 GX 9+1 270.370 -20.535 2.4 9.065 +1.162 5.4 0.49 10.9 0.0 0.00 0.0 SLX 1744-299_300 266.849 -30.017 2.7 359.277 -0.892 2.7 0.29 9.6 0.8 0.00 3.5 GX 3+1 267.010 -26.563 2.8 2.307 +0.773 3.2 0.33 9.5 0.0 0.00 0.0 SLX 1735-269 264.577 -26.947 3.6 0.839 +2.421 2.1 0.30 7.2 1.3 0.26 5.0 3A 1728-169 262.952 -16.934 4.2 8.546 +9.038 4.1 0.69 6.0 0.0 0.00 0.0 OAO 1657-415 255.185 -41.579 5.8 344.421 +0.378 7.2 1.72 4.2 0.0 0.00 0.0 IGR J18027-2016 270.643 -20.219 0.0 9.466 +1.096 2.1 0.00 4.7 0.0 0.00 0.0 GRS 1734-292 264.425 -29.076 0.0 358.967 +1.397 1.4 0.00 4.6 0.0 0.00 0.0 1A 1742-294 266.531 -29.475 6.0 359.597 -0.375 1.3 0.33 4.0 0.0 0.00 0.0 IGR J17456-2901 266.441 -28.999 5.5 359.962 -0.060 1.2 0.27 4.5 0.0 0.00 0.0 V2400 Oph 258.134 -24.277 5.6 359.832 +8.735 1.9 0.43 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 with 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 11.8 1.27 2.5 0.77 1A 1742-294 266.523 -29.515 359.559 -0.389 2.9 0.35 0.6 0.20 GX 3+1 266.983 -26.564 2.294 +0.794 28.6 0.58 3.9 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 76.4 1.99 21.5 1.12
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