INTEGRAL Galactic Bulge Monitoring Revolution 0788: Observation start 2009-03-28T08:06 = MJD 54918.338
Total Observation GTI = 12235 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 265.991 -29.748 0.9 359.119 -0.117 10.3 0.29 35.0 7.1 0.26 27.6 GX 1+4 263.010 -24.737 1.2 1.945 +4.799 8.8 0.34 25.6 0.0 0.00 0.0 Ginga 1826-24 277.363 -23.794 1.2 9.273 -6.083 14.0 0.56 25.0 5.4 0.45 11.9 GRS 1758-258 270.317 -25.742 1.3 4.516 -1.372 7.4 0.33 22.4 5.3 0.28 18.9 GX 5-1 270.286 -25.071 1.4 5.086 -1.016 7.5 0.36 20.9 0.0 0.00 0.0 H 1820-303 275.917 -30.362 1.8 2.786 -7.912 7.6 0.48 15.9 0.0 0.00 0.0 GX 349+2 256.416 -36.416 2.0 349.100 +2.765 7.8 0.57 13.6 0.0 0.00 0.0 4U 1722-30 261.869 -30.826 3.4 356.291 +2.299 2.5 0.33 7.5 1.5 0.00 5.4 GX 9+1 270.357 -20.512 3.9 9.078 +1.184 2.8 0.43 6.4 0.0 0.00 0.0 3A 1822-371 276.513 -37.072 3.6 356.905 -11.325 5.1 0.72 7.0 0.0 0.00 0.0 GX 13+1 273.613 -17.148 3.7 13.516 +0.126 4.9 0.73 6.8 0.0 0.00 0.0 XTE J1709-267 257.308 -26.668 4.1 357.426 +7.954 2.4 0.40 6.1 1.0 0.33 3.1 SLX 1744-299_300 266.820 -30.088 5.1 359.204 -0.907 1.5 0.30 4.9 0.0 0.00 0.0 MXB 1730-335 263.328 -33.392 4.4 354.827 -0.145 2.1 0.36 5.7 0.0 0.00 0.0 GX 17+2 274.005 -14.013 4.8 16.453 +1.290 8.1 1.56 5.2 0.0 0.00 0.0 SLX 1735-269 264.551 -27.019 4.6 0.766 +2.402 1.9 0.35 5.4 0.0 0.00 0.0 GX 3+1 266.943 -26.588 4.0 2.254 +0.812 1.9 0.31 6.2 0.0 0.00 0.0 OAO 1657-415 255.062 -41.640 6.1 344.317 +0.413 8.4 2.08 4.0 0.0 0.00 0.0 GX 354-0 262.912 -33.798 5.5 354.297 -0.076 1.6 0.36 4.5 0.0 0.00 0.0 Swift J174535.5-2901 266.404 -29.025 5.4 359.924 -0.045 1.5 0.33 4.6 0.0 0.00 0.0 1A 1742-294 266.537 -29.594 0.0 359.499 -0.441 1.3 0.00 4.2 0.0 0.00 0.0 3A 1728-169 262.892 -16.979 6.2 8.476 +9.063 2.4 0.62 3.9 0.0 0.00 0.0 1E 1743.1-2843 266.620 -28.679 5.8 0.318 -0.027 1.4 0.34 4.2 0.0 0.00 0.0 4U 1700-377 256.062 -37.802 6.2 347.824 +2.151 2.6 0.67 3.9 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 0.44 0.8 0.25 GX 3+1 266.983 -26.564 2.294 +0.794 29.5 0.52 3.6 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 104.2 1.95 11.4 0.84
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