INTEGRAL Galactic Bulge Monitoring Revolution 0789: Observation start 2009-03-30T10:14 = MJD 54920.427
Total Observation GTI = 11053 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 1700-377 255.983 -37.838 0.6 347.757 +2.179 57.9 0.91 63.9 16.6 0.71 23.4 GX 5-1 270.276 -25.079 0.8 5.074 -1.012 14.1 0.35 39.9 1.2 0.30 4.2 1E 1740.7-2942 265.984 -29.736 1.0 359.127 -0.105 10.5 0.34 30.8 7.2 0.30 24.3 GRS 1758-258 270.303 -25.743 1.2 4.509 -1.362 8.7 0.33 26.1 4.8 0.28 17.1 Ginga 1826-24 277.359 -23.797 1.2 9.269 -6.081 14.8 0.57 26.0 6.0 0.45 13.2 GX 1+4 263.011 -24.747 1.2 1.937 +4.793 10.2 0.40 25.4 0.0 0.00 0.0 H 1820-303 275.913 -30.356 2.0 2.791 -7.906 6.3 0.46 13.5 1.2 0.37 3.3 GX 349+2 256.433 -36.412 2.4 349.111 +2.757 8.0 0.73 11.0 0.0 0.00 0.0 GX 3+1 266.989 -26.542 3.4 2.315 +0.800 2.6 0.34 7.6 0.0 0.00 0.0 GX 9+1 270.358 -20.541 3.6 9.054 +1.169 3.1 0.44 7.1 0.0 0.00 0.0 GX 17+2 273.986 -14.058 3.2 16.404 +1.284 13.1 1.64 8.0 0.0 0.00 0.0 4U 1722-30 261.852 -30.777 3.5 356.323 +2.338 2.7 0.38 7.2 1.7 0.31 5.4 3A 1822-371 276.380 -37.118 4.6 356.816 -11.249 3.9 0.71 5.4 0.0 0.00 0.0 1E 1742.9-2849 266.555 -28.849 4.8 0.142 -0.067 1.8 0.34 5.2 0.0 0.00 0.0 SLX 1735-269 264.498 -27.032 4.7 0.729 +2.435 1.8 0.34 5.3 1.4 0.00 4.9 XTE J1709-267 257.335 -26.662 4.7 357.446 +7.938 2.7 0.51 5.3 0.0 0.00 0.0 3A 1728-169 262.923 -16.979 5.4 8.492 +9.038 3.3 0.72 4.6 0.0 0.00 0.0 NEW_1 269.649 -21.376 3.3 8.000 +1.329 3.5 0.44 7.9 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 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 4.4 0.50 0.7 0.27 GX 3+1 266.983 -26.564 2.294 +0.794 34.2 0.56 4.7 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 90.4 1.40 0.0 0.00
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