INTEGRAL Galactic Bulge Monitoring Revolution 0782: Observation start 2009-03-09T11:15 = MJD 54899.47
Total Observation GTI = 10247 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 1E 1740.7-2942 265.967 -29.739 0.9 359.116 -0.095 13.1 0.35 37.2 7.3 0.30 24.2 Ginga 1826-24 277.367 -23.793 1.3 9.276 -6.085 15.8 0.67 23.5 5.1 0.54 9.4 GX 354-0 262.975 -33.833 1.5 354.298 -0.139 8.0 0.43 18.5 0.0 0.00 0.0 GRS 1758-258 270.324 -25.739 1.8 4.522 -1.376 6.7 0.44 15.3 4.4 0.37 12.0 1A 1742-294 266.504 -29.514 1.8 359.551 -0.375 5.3 0.35 15.3 1.3 0.00 4.2 GX 1+4 263.004 -24.752 1.8 1.930 +4.795 7.0 0.46 15.2 0.0 0.00 0.0 H 1820-303 275.919 -30.351 2.2 2.797 -7.909 6.1 0.49 12.3 0.0 0.00 0.0 4U 1700-377 255.962 -37.847 2.3 347.741 +2.187 10.4 0.87 11.9 2.4 0.00 3.6 GX 17+2 274.022 -14.043 2.6 16.433 +1.261 26.5 2.65 10.0 0.0 0.00 0.0 GX 3+1 267.020 -26.541 3.3 2.330 +0.777 2.9 0.38 7.7 0.0 0.00 0.0 4U 1722-30 261.844 -30.816 3.2 356.287 +2.322 3.2 0.40 8.0 1.5 0.33 4.4 GX 5-1 270.275 -25.066 3.4 5.085 -1.005 3.3 0.44 7.5 0.0 0.00 0.0 GX 349+2 256.480 -36.412 3.7 349.134 +2.727 4.9 0.71 6.9 0.0 0.00 0.0 3A 1822-371 276.442 -37.094 3.8 356.859 -11.284 4.9 0.73 6.7 0.0 0.00 0.0 GX 9+1 270.408 -20.455 4.4 9.152 +1.171 3.1 0.54 5.6 0.0 0.00 0.0 SLX 1735-269 264.575 -26.966 4.8 0.821 +2.412 2.0 0.38 5.1 1.7 0.00 5.3JEM-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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.8 0.50 0.9 0.34 GX 3+1 266.983 -26.564 2.294 +0.794 25.8 0.72 3.3 0.37 GX 5-1 270.284 -25.079 5.077 -1.019 80.8 2.12 7.9 0.96
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