INTEGRAL Galactic Bulge Monitoring Revolution 0857: Observation start 2009-10-21T07:53 = MJD 55125.329
Total Observation GTI = 12347 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 1+4 263.015 -24.742 0.6 1.943 +4.792 23.7 0.34 69.8 0.0 0.00 0.0 4U 1700-377 255.983 -37.840 0.7 347.756 +2.178 38.4 0.81 47.5 8.5 0.64 13.4 1E 1740.7-2942 265.984 -29.740 0.9 359.123 -0.107 11.3 0.30 37.1 7.0 0.26 26.7 GX 5-1 270.286 -25.082 1.0 5.076 -1.021 10.5 0.34 30.5 0.0 0.00 0.0 GRS 1758-258 270.314 -25.734 1.2 4.521 -1.366 8.4 0.35 24.3 4.8 0.30 16.1 Ginga 1826-24 277.374 -23.803 1.3 9.269 -6.096 11.9 0.53 22.3 4.6 0.42 10.9 IGR J17586-2129 269.643 -21.426 2.2 7.954 +1.308 5.1 0.42 12.3 1.5 0.00 4.1 4U 1722-30 261.849 -30.795 2.8 356.306 +2.330 3.4 0.37 9.2 1.3 0.30 4.3 GX 9+1 270.332 -20.498 3.1 9.079 +1.212 3.7 0.45 8.3 0.0 0.00 0.0 H 1820-303 275.956 -30.368 3.6 2.797 -7.945 2.9 0.42 7.0 0.0 0.00 0.0 GX 349+2 256.410 -36.414 3.4 349.099 +2.770 5.2 0.69 7.4 0.0 0.00 0.0 3A 1822-371 276.436 -37.089 3.8 356.862 -11.277 4.0 0.60 6.6 0.0 0.00 0.0 SLX 1735-269 264.601 -27.004 3.8 0.802 +2.372 2.2 0.33 6.6 0.0 0.00 0.0 SLX 1744-299_300 266.897 -29.954 0.0 359.353 -0.895 1.7 0.00 5.7 0.0 0.00 0.0 GRS 1734-292 264.354 -29.194 5.2 358.833 +1.386 1.5 0.33 4.7 0.0 0.00 0.0 1E 1742.8-2853 266.463 -28.909 4.8 0.049 -0.029 1.6 0.31 5.1 0.0 0.00 0.0 IGR J17200-3116 259.999 -31.246 6.7 355.040 +3.386 1.4 0.38 3.6 0.0 0.00 0.0 1A 1742-294 266.617 -29.527 6.3 359.591 -0.465 1.2 0.32 3.9 0.0 0.00 0.0 GX 3+1 266.959 -26.552 5.9 2.292 +0.818 1.3 0.31 4.1 0.0 0.00 0.0 SGR 1806-20 272.171 -20.400 6.0 10.009 -0.242 1.9 0.47 4.1 0.0 0.00 0.0 GX 17+2 273.992 -14.032 5.9 16.430 +1.292 10.4 2.51 4.1 0.0 0.00 0.0 Oph Cluster 258.131 -23.450 6.2 0.515 +9.212 1.9 0.49 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 5.7 0.45 0.9 0.25 GX 3+1 266.983 -26.564 2.294 +0.794 34.3 0.59 3.9 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 132.2 1.85 18.2 0.85
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