INTEGRAL Galactic Bulge Monitoring Revolution 0552: Observation start 2007-04-21 = MJD 54211
Total Observation GTI = 12298 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 1700-377 255.987 -37.841 0.5 347.757 +2.175 52.4 0.65 80.7 14.5 0.51 28.5 GX 1+4 263.015 -24.742 0.7 1.943 +4.792 17.9 0.35 50.9 0.0 0.00 0.0 GRS 1758-258 270.308 -25.746 0.9 4.509 -1.367 13.0 0.35 36.8 8.9 0.29 30.6 Ginga 1826-24 277.383 -23.799 1.0 9.277 -6.101 17.3 0.52 33.3 7.1 0.40 17.6 1E 1740.7-2942 265.974 -29.739 1.4 359.119 -0.100 6.4 0.31 20.9 3.9 0.26 14.9 H 1820-303 275.929 -30.362 1.6 2.792 -7.922 7.8 0.45 17.6 0.0 0.00 0.0 GX 354-0 262.989 -33.839 1.9 354.298 -0.152 4.8 0.33 14.8 0.0 0.00 0.0 GX 349+2 256.424 -36.422 2.0 349.099 +2.756 8.4 0.60 14.0 0.0 0.00 0.0 GX 3+1 266.988 -26.591 2.4 2.273 +0.776 3.5 0.32 11.2 0.0 0.00 0.0 3A 1822-371 276.445 -37.121 2.4 356.836 -11.298 6.4 0.56 11.4 0.0 0.00 0.0 4U 1722-30 261.894 -30.818 2.2 356.309 +2.285 4.2 0.34 12.4 1.6 0.27 5.8 OAO 1657-415 255.220 -41.651 3.0 344.380 +0.312 13.2 1.50 8.8 0.0 0.00 0.0 GX 9+1 270.387 -20.555 3.1 9.055 +1.139 4.0 0.48 8.4 0.0 0.00 0.0 SLX 1744-299_300 266.922 -30.000 3.5 359.324 -0.937 2.3 0.31 7.3 0.9 0.26 3.4 SLX 1735-269 264.553 -26.944 4.5 0.830 +2.441 1.7 0.32 5.5 0.9 0.00 3.5 GRS 1734-292 264.362 -29.187 4.9 358.843 +1.384 1.5 0.30 5.0 0.9 0.25 3.7 GX 5-1 270.301 -25.140 5.0 5.032 -1.062 1.6 0.33 5.0 0.0 0.00 0.0 IGR J17456-2901 266.368 -28.975 0.0 359.950 +0.008 1.5 0.00 4.5 0.0 0.00 0.0 GX 17+2 274.035 -14.024 5.0 16.456 +1.258 19.9 4.04 4.9 0.0 0.00 0.0 1A 1742-294 266.553 -29.552 0.0 359.541 -0.431 1.2 0.00 3.9 0.0 0.00 0.0 3A 1728-169 262.955 -16.982 5.6 8.506 +9.010 3.3 0.76 4.4 0.0 0.00 0.0 1A 1743-288 266.744 -28.894 0.0 0.190 -0.232 1.1 0.00 3.5 0.0 0.00 0.0 SAX J1818.6-1703 274.659 -16.856 7.5 14.249 -0.615 3.4 1.08 3.2 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 12.3 1.41 3.0 0.92 1A 1742-294 266.523 -29.515 359.559 -0.389 2.7 0.36 0.4 0.18 GX 3+1 266.983 -26.564 2.294 +0.794 25.3 0.58 4.0 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 57.0 1.71 3.1 0.69
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