INTEGRAL Galactic Bulge Monitoring Revolution 0549: Observation start 2007-04-12 = MJD 54202
Total Observation GTI = 9759 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 1700-377 255.981 -37.843 0.8 347.753 +2.178 29.8 0.74 40.1 7.4 0.59 12.5 GX 1+4 263.011 -24.748 0.8 1.936 +4.792 14.2 0.37 38.6 0.0 0.00 0.0 GX 354-0 262.983 -33.829 0.9 354.304 -0.143 13.1 0.37 35.4 2.3 0.31 7.3 GRS 1758-258 270.301 -25.736 1.0 4.513 -1.357 13.0 0.39 33.0 9.0 0.33 27.2 Ginga 1826-24 277.378 -23.803 1.1 9.272 -6.099 17.5 0.63 27.9 6.1 0.50 12.1 1E 1740.7-2942 265.984 -29.742 1.1 359.121 -0.108 8.8 0.32 27.2 5.2 0.28 18.3 1A 1742-294 266.511 -29.497 1.4 359.569 -0.371 6.7 0.34 19.9 2.6 0.00 9.0 H 1820-303 275.937 -30.360 2.1 2.797 -7.927 6.1 0.47 12.9 0.0 0.00 0.0 GX 349+2 256.418 -36.395 2.1 349.118 +2.776 8.5 0.66 12.8 0.0 0.00 0.0 GX 3+1 266.975 -26.553 2.7 2.299 +0.805 3.4 0.34 9.8 0.0 0.00 0.0 4U 1722-30 261.902 -30.771 2.5 356.352 +2.305 4.0 0.37 10.8 2.0 0.31 6.5 GX 9+1 270.414 -20.506 2.9 9.110 +1.141 4.3 0.47 9.1 0.0 0.00 0.0 3A 1822-371 276.427 -37.114 2.9 356.836 -11.282 6.5 0.73 8.9 0.0 0.00 0.0 GX 5-1 270.247 -25.077 2.9 5.063 -0.988 3.3 0.36 9.1 1.3 0.30 4.3 SLX 1744-299_300 266.817 -30.027 0.0 359.254 -0.873 2.1 0.00 6.2 0.0 0.00 0.0 SLX 1735-269 264.600 -27.002 3.9 0.803 +2.374 2.2 0.33 6.4 1.4 0.29 4.9 OAO 1657-415 255.215 -41.674 3.7 344.360 +0.301 13.4 1.95 6.9 0.0 0.00 0.0 3A 1728-169 263.005 -16.940 4.6 8.568 +8.992 4.0 0.74 5.4 0.0 0.00 0.0 IGR J17252-3616 261.304 -36.310 4.9 351.478 -0.374 2.3 0.46 5.1 0.0 0.00 0.0 AX J1749.2-2725 267.337 -27.456 6.3 1.692 +0.064 1.2 0.31 3.8 0.0 0.00 0.0 1E 1742.9-2849 266.523 -28.795 0.0 0.174 -0.015 1.4 0.00 4.2 0.0 0.00 0.0 NEW_1 284.668 -39.641 4.1 357.053 -18.212 29.8 4.72 6.2 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 7.7 1.25 2.4 0.87 GX 3+1 266.983 -26.564 2.294 +0.794 32.6 0.57 4.4 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 76.3 2.12 5.7 0.88
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