INTEGRAL Galactic Bulge Monitoring Revolution 0671: Observation start 2008-04-11T16:16 = MJD 54567.679
Total Observation GTI = 12239 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17473-2721 266.822 -27.342 0.4 1.553 +0.514 38.2 0.32 119.5 16.8 0.26 64.0 4U 1700-377 255.983 -37.846 0.5 347.751 +2.175 62.3 0.70 89.1 20.6 0.53 39.1 GRO J1750-27 267.285 -26.646 0.7 2.363 +0.520 15.4 0.32 47.8 0.0 0.00 0.0 4U 1722-30 261.891 -30.797 1.1 356.325 +2.299 9.6 0.34 28.3 3.8 0.27 13.8 Ginga 1826-24 277.367 -23.809 1.2 9.261 -6.093 16.3 0.64 25.6 6.7 0.48 14.0 SAX J1750.8-2900 267.605 -29.038 1.4 0.455 -0.951 6.9 0.32 21.3 2.9 0.26 10.9 GRS 1758-258 270.309 -25.734 1.5 4.519 -1.362 7.1 0.37 19.1 4.8 0.30 16.2 H 1820-303 275.915 -30.369 1.6 2.780 -7.914 8.4 0.47 17.7 0.0 0.00 0.0 XTE J1810-189 272.589 -19.065 1.8 11.368 +0.060 9.9 0.64 15.4 4.6 0.50 9.2 1E 1740.7-2942 265.998 -29.733 1.8 359.135 -0.114 4.9 0.31 15.9 2.5 0.25 10.1 GX 349+2 256.414 -36.412 2.3 349.102 +2.768 6.9 0.60 11.5 0.0 0.00 0.0 GX 354-0 262.984 -33.845 2.8 354.291 -0.152 3.3 0.36 9.3 1.0 0.00 3.6 3A 1822-371 276.469 -37.089 2.9 356.873 -11.301 6.1 0.68 8.9 0.0 0.00 0.0 XTE J1709-267 257.400 -26.628 2.8 357.507 +7.911 3.9 0.42 9.3 1.4 0.32 4.2 SLX 1735-269 264.612 -26.988 3.7 0.821 +2.373 2.2 0.32 6.8 0.0 0.00 0.0 GX 3+1 266.875 -26.572 3.7 2.236 +0.872 2.3 0.00 6.8 0.0 0.00 0.0 GX 9+1 270.389 -20.538 3.4 9.071 +1.145 3.3 0.45 7.5 0.0 0.00 0.0 OAO 1657-415 255.192 -41.702 3.9 344.328 +0.297 12.2 1.87 6.5 0.0 0.00 0.0 GX 5-1 270.208 -25.057 4.7 5.062 -0.947 1.9 0.36 5.3 0.0 0.00 0.0 SLX 1744-299_300 266.817 -30.027 0.0 359.254 -0.873 1.7 0.00 5.3 0.0 0.00 0.0 IGR J17456-2901 266.410 -28.932 5.3 0.006 -0.002 1.5 0.32 4.7 1.0 0.26 3.8 3A 1728-169 262.930 -16.996 5.5 8.482 +9.023 3.0 0.69 4.4 0.0 0.00 0.0 GX 13+1 273.621 -17.174 5.0 13.497 +0.107 4.0 0.82 4.9 0.0 0.00 0.0 GX 1+4 263.034 -24.718 7.1 1.973 +4.790 1.1 0.33 3.4 0.0 0.00 0.0 IGR J17252-3616 261.280 -36.207 5.4 351.552 -0.300 2.0 0.43 4.5 0.0 0.00 0.0 1A 1742-294 266.434 -29.536 0.0 359.501 -0.334 1.2 0.00 3.7 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 10.3 1.37 2.4 0.92 1A 1742-294 266.523 -29.515 359.559 -0.389 3.6 0.43 0.7 0.24 IGR J17473-2721 266.825 -27.344 1.553 +0.510 8.6 0.49 4.9 0.30 GX 3+1 266.983 -26.564 2.294 +0.794 39.4 0.63 0.0 0.00 GX 5-1 270.284 -25.079 5.077 -1.019 78.0 2.46 3.9 1.01 GRO J1750-27 267.303 -26.643 2.373 +0.508 3.9 0.52 3.6 0.33
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