INTEGRAL Galactic Bulge Monitoring Revolution 0722: Observation start 2008-09-10T23:41 = MJD 54719.988
Total Observation GTI = 10439 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 354-0 262.994 -33.835 0.8 354.305 -0.154 17.5 0.40 43.7 4.3 0.33 13.0 GX 5-1 270.287 -25.085 0.9 5.073 -1.023 15.1 0.42 35.9 0.0 0.00 0.0 GRS 1758-258 270.306 -25.753 1.0 4.501 -1.370 12.7 0.42 30.2 7.4 0.35 21.3 IGR J17473-2721 266.827 -27.335 1.1 1.562 +0.514 9.1 0.31 29.1 3.9 0.27 14.4 Ginga 1826-24 277.351 -23.798 1.1 9.265 -6.075 17.4 0.61 28.3 6.9 0.49 14.1 1E 1740.7-2942 265.979 -29.756 1.2 359.107 -0.112 7.9 0.32 24.7 5.1 0.27 18.8 H 1820-303 275.911 -30.362 1.6 2.784 -7.908 8.1 0.47 17.3 0.0 0.00 0.0 GX 1+4 262.998 -24.740 1.6 1.936 +4.807 7.5 0.43 17.4 0.0 0.00 0.0 4U 1700-377 255.977 -37.827 2.1 347.763 +2.189 10.6 0.81 13.1 0.0 0.00 0.0 GX 349+2 256.453 -36.409 2.3 349.123 +2.745 8.1 0.68 11.9 0.0 0.00 0.0 4U 1722-30 261.853 -30.815 2.3 356.292 +2.316 4.5 0.39 11.6 1.4 0.31 4.3 OAO 1657-415 255.210 -41.658 2.4 344.370 +0.314 19.1 1.71 11.2 0.0 0.00 0.0 GX 3+1 267.019 -26.574 2.5 2.302 +0.761 3.5 0.33 10.5 0.0 0.00 0.0 GX 9+1 270.399 -20.527 2.7 9.086 +1.143 4.9 0.50 9.8 0.0 0.00 0.0 3A 1822-371 276.460 -37.078 3.2 356.880 -11.290 5.3 0.65 8.1 0.0 0.00 0.0 SLX 1735-269 264.559 -27.000 3.9 0.785 +2.407 2.2 0.34 6.5 0.0 0.00 0.0 H 1702-429 256.546 -43.126 4.2 343.807 -1.363 17.6 2.92 6.0 8.9 2.05 4.3 IGR J17252-3616 261.238 -36.286 4.7 351.468 -0.316 2.5 0.47 5.3 0.0 0.00 0.0 1E 1742.8-2853 266.506 -28.974 5.2 0.014 -0.095 1.5 0.31 4.8 0.0 0.00 0.0 NEW_1 279.648 -16.653 4.8 16.642 -4.756 9.8 1.89 5.2 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 4U 1722-30 261.888 -30.802 356.320 +2.298 7.0 0.96 1.2 0.60 1A 1742-294 266.523 -29.515 359.559 -0.389 4.3 0.47 1.0 0.26 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.4 0.45 0.7 0.30 GX 3+1 266.983 -26.564 2.294 +0.794 47.7 0.78 6.8 0.39 GX 5-1 270.284 -25.079 5.077 -1.019 129.3 2.73 19.1 1.25
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