INTEGRAL Galactic Bulge Monitoring Revolution 0540: Observation start 2007-03-16 = MJD 54175
Total Observation GTI = 24560 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 -33.829 0.4 354.306 -0.146 33.0 0.23 141.6 9.5 0.19 50.4 GX 1+4 263.010 -24.749 0.5 1.935 +4.792 23.6 0.25 93.8 0.0 0.00 0.0 1E 1740.7-2942 265.984 -29.748 0.7 359.116 -0.111 11.6 0.22 51.7 6.8 0.19 36.1 GRS 1758-258 270.300 -25.747 0.7 4.504 -1.361 11.9 0.23 50.6 8.1 0.19 43.3 4U 1700-377 255.988 -37.847 0.7 347.753 +2.171 20.9 0.44 47.4 5.6 0.34 16.2 Ginga 1826-24 277.356 -23.802 0.8 9.263 -6.081 18.7 0.48 39.1 6.5 0.36 17.7 GX 349+2 256.437 -36.417 1.0 349.109 +2.751 11.4 0.36 32.0 0.0 0.00 0.0 H 1820-303 275.899 -30.353 1.2 2.788 -7.894 8.4 0.34 25.0 0.0 0.00 0.0 1A 1742-294 266.510 -29.514 1.4 359.555 -0.379 4.5 0.22 20.1 1.3 0.19 7.2 GRS 1741.9-2853 266.292 -28.933 1.8 359.951 +0.086 3.4 0.22 15.0 2.1 0.19 11.1 GX 5-1 270.293 -25.079 1.6 5.081 -1.026 4.4 0.25 17.7 0.0 0.00 0.0 GX 3+1 266.995 -26.568 1.7 2.295 +0.782 4.1 0.24 17.0 0.0 0.00 0.0 4U 1722-30 261.865 -30.789 1.7 356.319 +2.322 4.0 0.23 16.9 1.5 0.19 7.9 3A 1822-371 276.461 -37.094 1.6 356.866 -11.298 8.1 0.46 17.5 0.0 0.00 0.0 OAO 1657-415 255.220 -41.668 2.1 344.367 +0.302 10.4 0.79 13.2 3.1 0.59 5.2 SLX 1735-269 264.569 -27.017 3.3 0.776 +2.390 1.8 0.24 7.8 1.1 0.20 5.3 1E 1743.1-2843 266.669 -28.751 0.0 0.279 -0.101 1.5 0.00 6.7 0.0 0.00 0.0 4U 1735-444 264.597 -44.446 4.5 346.003 -6.903 8.3 1.48 5.6 0.0 0.00 0.0 GX 9+1 270.388 -20.522 4.1 9.085 +1.155 2.2 0.35 6.2 0.0 0.00 0.0 SLX 1744-299_300 266.862 -29.998 5.0 359.299 -0.892 1.1 0.22 4.9 0.0 0.00 0.0 3A 1728-169 262.901 -16.853 5.2 8.589 +9.122 2.8 0.59 4.8 0.0 0.00 0.0 GX 17+2 274.053 -14.019 4.6 16.469 +1.245 12.5 2.29 5.5 0.0 0.00 0.0 GRS 1734-292 264.379 -29.158 4.8 358.876 +1.386 1.2 0.23 5.2 0.0 0.00 0.0 XB 1832-330 278.886 -32.984 4.4 1.521 -11.333 2.7 0.48 5.6 1.6 0.36 4.5 SAX J1712.6-3739 258.173 -37.692 5.8 348.910 +0.879 1.5 0.00 4.2 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.4 0.26 1.1 0.16 GX 354-0 262.989 -33.835 354.302 -0.150 11.2 0.69 4.8 0.49 1A 1742-294 266.523 -29.515 359.559 -0.389 1.5 0.25 0.7 0.18 GX 3+1 266.983 -26.564 2.294 +0.794 33.8 0.50 4.9 0.26 GX 5-1 270.284 -25.079 5.077 -1.019 69.1 2.91 6.1 1.30 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.6 0.30 0.4 0.23
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