INTEGRAL Galactic Bulge Monitoring Revolution 0791: Observation start 2009-04-05T23:30 = MJD 54926.98
Total Observation GTI = 12361 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 1700-377 255.991 -37.840 0.7 347.760 +2.173 35.1 0.76 46.2 7.2 0.61 11.9 1E 1740.7-2942 265.972 -29.741 1.0 359.117 -0.099 10.6 0.32 32.9 7.6 0.28 26.8 Ginga 1826-24 277.360 -23.792 1.1 9.273 -6.079 14.6 0.52 28.1 5.7 0.43 13.4 GX 1+4 263.015 -24.740 1.2 1.945 +4.794 9.6 0.37 26.1 0.0 0.00 0.0 GRS 1758-258 270.311 -25.750 1.2 4.506 -1.372 8.3 0.32 26.1 5.5 0.27 20.1 H 1820-303 275.925 -30.381 1.9 2.773 -7.927 6.2 0.42 14.6 1.7 0.35 5.0 GX 349+2 256.436 -36.423 1.8 349.104 +2.748 9.8 0.64 15.4 0.0 0.00 0.0 GX 5-1 270.295 -25.084 1.9 5.078 -1.029 4.7 0.32 14.6 0.0 0.00 0.0 GX 9+1 270.394 -20.535 2.4 9.076 +1.143 4.8 0.43 11.1 0.0 0.00 0.0 OAO 1657-415 255.219 -41.663 2.3 344.371 +0.306 21.0 1.79 11.7 5.4 1.39 3.9 GX 17+2 274.013 -14.027 2.7 16.444 +1.275 23.4 2.38 9.8 0.0 0.00 0.0 3A 1822-371 276.458 -37.026 3.5 356.928 -11.265 3.8 0.53 7.3 0.0 0.00 0.0 GX 354-0 263.033 -33.820 3.1 354.335 -0.173 2.9 0.34 8.4 0.0 0.00 0.0 GX 3+1 266.981 -26.558 2.7 2.298 +0.798 3.1 0.32 9.7 0.0 0.00 0.0 IGR J17252-3616 261.296 -36.316 3.4 351.468 -0.372 3.4 0.46 7.5 0.0 0.00 0.0 4U 1722-30 261.893 -30.804 3.5 356.320 +2.293 2.7 0.37 7.2 1.4 0.00 4.5 GX 13+1 273.631 -17.206 4.0 13.474 +0.083 4.7 0.75 6.3 0.0 0.00 0.0 XTE J1709-267 257.365 -26.672 4.7 357.453 +7.911 2.6 0.49 5.2 0.0 0.00 0.0 NEW_0365 250.488 -34.334 5.0 347.682 +7.834 6.7 1.37 4.9 0.0 0.00 0.0 SLX 1744-299_300 266.799 -29.924 7.2 359.334 -0.806 1.1 0.34 3.3 0.0 0.00 0.0 SLX 1735-269 264.589 -26.975 5.2 0.821 +2.397 1.6 0.34 4.7 0.0 0.00 0.0 3A 1728-169 263.020 -16.935 5.5 8.580 +8.982 3.3 0.74 4.5 0.0 0.00 0.0 XB 1832-330 278.949 -33.012 6.5 1.518 -11.393 2.0 0.00 3.7 0.0 0.00 0.0 1E 1742.8-2853 266.480 -28.889 6.8 0.074 -0.032 1.1 0.31 3.6 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 3.8 0.41 0.6 0.25 GX 3+1 266.983 -26.564 2.294 +0.794 33.9 0.62 4.6 0.32 GX 5-1 270.284 -25.079 5.077 -1.019 77.2 1.41 5.5 0.59
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