INTEGRAL Galactic Bulge Monitoring Revolution 0847: Observation start 2009-09-19T21:52 = MJD 55093.912
Total Observation GTI = 11937 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 1700-377 255.979 -37.843 0.4 347.751 +2.178 82.1 0.82 100.0 19.2 0.63 30.3 1E 1740.7-2942 265.982 -29.743 0.9 359.119 -0.107 11.9 0.35 34.0 7.2 0.30 24.0 GX 5-1 270.282 -25.076 1.0 5.079 -1.016 11.6 0.38 30.9 0.0 0.00 0.0 GRS 1758-258 270.293 -25.749 1.1 4.499 -1.357 10.3 0.38 26.7 4.7 0.32 14.6 Ginga 1826-24 277.367 -23.794 1.2 9.275 -6.086 13.6 0.54 25.3 4.8 0.43 11.3 GX 1+4 263.002 -24.739 1.5 1.939 +4.803 7.1 0.37 19.2 0.0 0.00 0.0 GX 349+2 256.428 -36.417 1.6 349.105 +2.757 12.7 0.70 18.2 0.0 0.00 0.0 IGR J17511-3057 267.792 -30.965 1.7 358.882 -2.076 5.9 0.36 16.4 2.2 0.31 7.1 IGR J17586-2129 269.620 -21.350 2.3 8.009 +1.366 4.9 0.43 11.5 0.0 0.00 0.0 H 1820-303 275.904 -30.362 2.3 2.782 -7.902 5.1 0.45 11.5 0.0 0.00 0.0 GX 17+2 274.014 -14.015 2.6 16.455 +1.280 15.2 1.49 10.2 0.0 0.00 0.0 4U 1722-30 261.909 -30.798 3.5 356.333 +2.286 2.9 0.39 7.4 1.8 0.32 5.7 3A 1822-371 276.399 -37.025 4.5 356.907 -11.223 4.1 0.74 5.5 0.0 0.00 0.0 GX 3+1 266.964 -26.584 3.7 2.268 +0.798 2.2 0.33 6.8 0.0 0.00 0.0 SLX 1735-269 264.591 -26.981 3.8 0.817 +2.392 2.3 0.35 6.7 0.0 0.00 0.0 IGR J17252-3616 261.334 -36.204 4.7 351.578 -0.334 2.6 0.49 5.3 0.0 0.00 0.0 1E 1742.9-2849 266.518 -28.856 4.6 0.120 -0.042 1.7 0.31 5.4 0.0 0.00 0.0 SLX 1744-299_300 266.843 -30.019 5.7 359.273 -0.888 1.5 0.36 4.3 0.0 0.00 0.0 OAO 1657-415 255.105 -41.688 5.3 344.299 +0.358 10.3 2.21 4.7 0.0 0.00 0.0 GRS 1734-292 264.332 -29.056 5.4 358.940 +1.476 1.6 0.35 4.5 0.0 0.00 0.0 GX 354-0 262.879 -33.811 5.7 354.272 -0.061 1.8 0.42 4.3 1.4 0.34 4.2JEM-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 6.3 0.51 0.8 0.26 GX 3+1 266.983 -26.564 2.294 +0.794 26.6 0.57 2.2 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 121.7 1.66 10.3 0.68
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