INTEGRAL Galactic Bulge Monitoring Revolution 0604: Observation start 2007-09-24 = MJD 54367
Total Observation GTI = 12325 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.984 -37.848 0.5 347.750 +2.173 41.7 0.56 74.7 12.5 0.44 28.2 GX 1+4 263.009 -24.747 0.8 1.936 +4.794 15.9 0.35 45.2 0.0 0.00 0.0 Ginga 1826-24 277.366 -23.791 1.0 9.277 -6.084 19.6 0.64 30.7 7.0 0.49 14.2 SAX J1810.8-2609 272.688 -26.136 1.2 5.211 -3.426 9.5 0.37 25.6 4.6 0.30 15.6 H 1820-303 275.926 -30.360 1.2 2.792 -7.919 11.0 0.45 24.6 0.0 0.00 0.0 GX 354-0 262.988 -33.825 1.4 354.310 -0.144 6.5 0.31 21.0 0.0 0.00 0.0 GX 5-1 270.261 -25.084 1.5 5.063 -1.003 6.6 0.36 18.5 0.0 0.00 0.0 GX 349+2 256.428 -36.436 1.6 349.089 +2.745 8.6 0.48 17.6 0.0 0.00 0.0 GX 3+1 266.969 -26.561 1.8 2.290 +0.806 5.5 0.34 15.9 0.0 0.00 0.0 GRS 1758-258 270.315 -25.745 2.2 4.512 -1.373 4.0 0.32 12.3 1.8 0.26 6.8 3A 1822-371 276.435 -37.102 2.0 356.850 -11.282 7.5 0.55 13.5 0.0 0.00 0.0 SLX 1744-299_300 266.863 -30.041 2.4 359.263 -0.915 3.1 0.28 11.0 1.2 0.24 5.1 GX 9+1 270.395 -20.540 2.5 9.072 +1.140 5.8 0.55 10.6 0.0 0.00 0.0 H 1702-429 256.537 -43.030 3.1 343.880 -1.299 11.9 1.41 8.5 0.0 0.00 0.0 4U 1722-30 261.889 -30.803 3.3 356.319 +2.297 2.9 0.38 7.7 1.8 0.31 5.8 SAX J1712.6-3739 258.038 -37.650 4.0 348.881 +0.990 2.9 0.46 6.4 0.0 0.00 0.0 IGR J17252-3616 261.282 -36.278 3.9 351.494 -0.341 2.4 0.37 6.5 0.0 0.00 0.0 SLX 1735-269 264.559 -26.984 3.8 0.799 +2.415 2.2 0.34 6.6 0.0 0.00 0.0 GRS 1734-292 264.456 -29.161 4.8 358.909 +1.328 1.7 0.33 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 5.8 0.70 1.7 0.50 1A 1742-294 266.523 -29.515 359.559 -0.389 3.4 0.36 0.5 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 37.0 0.81 6.1 0.43 GX 5-1 270.284 -25.079 5.077 -1.019 51.9 4.06 4.2 1.85
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