INTEGRAL Galactic Bulge Monitoring Revolution 0780: Observation start 2009-03-03T11:42 = MJD 54893.488
Total Observation GTI = 11906 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 1E 1740.7-2942 265.970 -29.753 0.8 359.105 -0.103 12.1 0.29 41.3 7.3 0.26 28.3 4U 1700-377 255.984 -37.846 0.8 347.752 +2.174 26.9 0.65 41.2 6.1 0.52 11.7 GX 5-1 270.279 -25.076 0.9 5.078 -1.013 11.2 0.33 34.1 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.791 1.1 9.280 -6.089 17.1 0.63 27.4 6.6 0.50 13.2 GX 349+2 256.427 -36.418 1.3 349.103 +2.757 12.9 0.54 23.7 0.0 0.00 0.0 GX 354-0 262.990 -33.831 1.5 354.306 -0.149 7.0 0.35 19.7 1.8 0.30 6.1 GRS 1758-258 270.293 -25.736 1.6 4.510 -1.351 5.7 0.32 18.0 4.1 0.27 15.1 H 1820-303 275.888 -30.353 1.7 2.783 -7.886 8.0 0.47 16.9 0.0 0.00 0.0 1A 1742-294 266.532 -29.534 2.0 359.547 -0.406 4.1 0.29 14.1 1.3 0.26 5.2 OAO 1657-415 255.191 -41.631 2.1 344.383 +0.343 15.9 1.20 13.2 0.0 0.00 0.0 4U 1722-30 261.876 -30.791 2.4 356.323 +2.313 3.7 0.33 11.2 1.4 0.28 5.0 GX 1+4 262.998 -24.750 2.5 1.928 +4.801 4.2 0.40 10.7 0.0 0.00 0.0 GX 3+1 267.058 -26.548 2.9 2.341 +0.744 2.9 0.32 9.0 0.0 0.00 0.0 3A 1822-371 276.443 -37.116 2.8 356.839 -11.294 5.3 0.58 9.2 0.0 0.00 0.0 SLX 1744-299_300 266.810 -30.014 3.1 359.262 -0.861 2.4 0.29 8.2 0.0 0.00 0.0 SLX 1735-269 264.546 -27.000 3.1 0.779 +2.417 2.7 0.32 8.3 1.6 0.28 5.8 GX 9+1 270.395 -20.575 4.7 9.042 +1.123 2.7 0.00 5.3 0.0 0.00 0.0 IGR J17391-3021 264.784 -30.413 5.4 358.003 +0.419 1.4 0.00 4.5 0.0 0.00 0.0 1E 1742.8-2853 266.441 -28.939 7.6 0.014 -0.028 0.9 0.30 3.1 0.0 0.00 0.0 IGR J18027-2016 270.734 -20.406 0.0 9.345 +0.930 2.1 0.00 4.0 0.0 0.00 0.0 IGR J17252-3616 261.261 -36.211 5.0 351.540 -0.289 2.1 0.42 5.0 0.0 0.00 0.0 NEW_1 272.390 -22.229 3.9 8.507 -1.307 3.0 0.46 6.5 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 10.1 1.20 2.8 0.85 1A 1742-294 266.523 -29.515 359.559 -0.389 1.7 0.33 0.7 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 31.6 0.72 4.3 0.38 GX 5-1 270.284 -25.079 5.077 -1.019 104.4 2.77 14.2 1.22
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