INTEGRAL Galactic Bulge Monitoring Revolution 0610: Observation start 2007-10-11 = MJD 54384
Total Observation GTI = 12405 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 1700-377 255.989 -37.844 0.6 347.756 +2.172 49.3 0.74 67.0 15.1 0.57 26.5 GX 1+4 263.011 -24.748 0.8 1.936 +4.792 16.3 0.36 45.0 0.0 0.00 0.0 Ginga 1826-24 277.367 -23.791 0.8 9.278 -6.085 20.5 0.53 38.8 7.8 0.42 18.5 SAX J1810.8-2609 272.698 -26.151 1.2 5.202 -3.441 9.3 0.36 25.8 3.4 0.30 11.5 GX 5-1 270.287 -25.085 1.3 5.074 -1.024 7.7 0.33 23.5 0.0 0.00 0.0 H 1820-303 275.925 -30.351 1.4 2.800 -7.914 8.2 0.41 20.1 0.0 0.00 0.0 GX 354-0 262.983 -33.845 1.5 354.291 -0.152 6.3 0.34 18.8 0.0 0.00 0.0 GRS 1758-258 270.278 -25.748 1.8 4.493 -1.345 4.9 0.31 15.5 2.5 0.26 9.6 OAO 1657-415 255.209 -41.645 2.0 344.380 +0.323 30.2 2.14 14.1 9.9 1.51 6.5 3A 1822-371 276.442 -37.112 1.8 356.843 -11.292 9.0 0.59 15.1 2.3 0.47 4.8 GX 3+1 266.972 -26.553 2.0 2.298 +0.808 4.1 0.30 13.4 0.0 0.00 0.0 GX 349+2 256.464 -36.409 2.1 349.128 +2.739 8.0 0.60 13.2 0.0 0.00 0.0 GX 9+1 270.376 -20.560 2.1 9.046 +1.145 5.6 0.43 12.8 0.0 0.00 0.0 SLX 1744-299_300 266.857 -30.002 2.5 359.294 -0.890 3.1 0.29 10.9 1.4 0.25 5.8 SLX 1735-269 264.616 -26.981 2.8 0.829 +2.374 3.1 0.33 9.3 1.7 0.28 6.2 1A 1743-288 266.800 -28.955 0.0 0.164 -0.304 2.5 0.00 9.0 1.3 0.24 5.5 4U 1722-30 261.837 -30.818 2.9 356.282 +2.326 3.2 0.35 8.9 1.3 0.29 4.6 GX 13+1 273.643 -17.129 3.0 13.547 +0.110 6.3 0.73 8.7 0.0 0.00 0.0 Swift J174535.5-2901 266.423 -29.035 0.0 359.923 -0.065 1.7 0.00 5.7 0.0 0.00 0.0 GX 17+2 274.033 -14.075 4.2 16.410 +1.236 12.8 2.12 6.0 0.0 0.00 0.0 IGR J17091-3624 257.212 -36.390 0.0 349.506 +2.268 2.5 0.00 4.4 0.0 0.00 0.0 QSO B1730-130 263.169 -13.113 5.8 11.957 +10.871 10.1 2.39 4.2 0.0 0.00 0.0 IGR J17200-3116 260.080 -31.313 6.2 355.025 +3.292 1.5 0.00 3.9 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 10.4 2.06 2.9 1.21 1A 1742-294 266.523 -29.515 359.559 -0.389 4.0 0.46 0.9 0.28 GX 3+1 266.983 -26.564 2.294 +0.794 35.0 0.61 4.9 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 84.3 1.70 9.4 0.74 SLX 1746-331 267.461 -33.199 356.816 -2.976 6.3 0.77 0.0 0.00
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