INTEGRAL Galactic Bulge Monitoring Revolution 0611: Observation start 2007-10-14 = MJD 54387
Total Observation GTI = 12294 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 1+4 263.019 -24.742 0.8 1.945 +4.790 14.9 0.34 44.5 0.0 0.00 0.0 4U 1700-377 255.988 -37.838 0.9 347.760 +2.176 27.0 0.72 37.5 9.3 0.57 16.3 Ginga 1826-24 277.365 -23.788 0.9 9.279 -6.082 19.7 0.56 34.9 8.3 0.45 18.5 GX 354-0 262.985 -33.825 1.0 354.309 -0.142 11.4 0.36 31.6 1.9 0.30 6.2 SAX J1810.8-2609 272.699 -26.166 1.3 5.190 -3.449 8.8 0.37 23.6 4.3 0.31 14.1 GX 5-1 270.286 -25.069 1.5 5.087 -1.014 6.6 0.34 19.3 0.0 0.00 0.0 H 1820-303 275.917 -30.355 1.6 2.793 -7.910 8.0 0.45 17.6 0.0 0.00 0.0 GX 3+1 266.971 -26.555 1.9 2.296 +0.808 4.5 0.30 14.7 0.0 0.00 0.0 GRS 1758-258 270.310 -25.750 2.1 4.506 -1.371 4.3 0.34 12.7 2.6 0.28 9.2 3A 1822-371 276.437 -37.095 2.1 356.857 -11.281 7.5 0.59 12.8 0.0 0.00 0.0 GX 349+2 256.448 -36.405 2.4 349.124 +2.751 7.0 0.62 11.3 0.0 0.00 0.0 4U 1722-30 261.888 -30.808 2.6 356.314 +2.295 3.5 0.35 10.0 1.5 0.28 5.4 SLX 1735-269 264.572 -26.969 3.3 0.817 +2.413 2.5 0.32 7.9 0.0 0.00 0.0 IGR J17252-3616 261.300 -36.280 2.9 351.500 -0.354 3.8 0.43 8.9 0.0 0.00 0.0 IGR J17091-3624 257.321 -36.394 3.7 349.554 +2.195 3.8 0.57 6.8 2.7 0.45 6.1 GX 9+1 270.444 -20.519 3.8 9.113 +1.110 3.0 0.45 6.6 0.0 0.00 0.0 SLX 1744-299_300 266.912 -30.021 4.2 359.302 -0.940 1.9 0.32 5.9 0.0 0.00 0.0 1A 1742-294 266.494 -29.553 4.7 359.514 -0.387 1.6 0.30 5.3 0.0 0.00 0.0 3A 1728-169 262.822 -16.978 6.1 8.441 +9.120 3.1 0.76 4.0 0.0 0.00 0.0 SLX 1737-282 265.273 -28.340 6.7 359.986 +1.158 1.1 0.29 3.6 0.0 0.00 0.0 XTE J1710-281 257.535 -28.122 5.3 356.356 +6.940 2.0 0.43 4.7 0.0 0.00 0.0 GRS 1741.9-2853 266.378 -28.882 0.0 0.034 +0.048 1.3 0.00 3.8 0.0 0.00 0.0 IGR J18027-1455 270.691 -14.952 7.4 14.078 +3.647 5.8 1.77 3.2 0.0 0.00 0.0 NEW_1 266.848 -29.048 0.0 0.105 -0.389 1.9 0.00 6.3 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 4.7 0.43 0.8 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 34.2 0.67 5.5 0.34 GX 5-1 270.284 -25.079 5.077 -1.019 82.0 2.07 7.2 0.85 SLX 1746-331 267.461 -33.199 356.816 -2.976 5.0 0.60 0.0 0.00
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