INTEGRAL Galactic Bulge Monitoring Revolution 0786: Observation start 2009-03-21T16:44 = MJD 54911.698
Total Observation GTI = 12376 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 265.976 -29.742 0.9 359.117 -0.102 11.9 0.34 35.2 6.8 0.31 22.2 GX 1+4 263.019 -24.746 1.2 1.942 +4.787 7.4 0.31 23.9 0.0 0.00 0.0 Ginga 1826-24 277.373 -23.799 1.4 9.273 -6.093 13.8 0.65 21.3 4.0 0.53 7.6 GRS 1758-258 270.296 -25.743 1.4 4.506 -1.356 7.6 0.36 21.1 4.1 0.30 13.5 1A 1742-294 266.509 -29.506 1.3 359.560 -0.374 7.0 0.31 22.5 1.7 0.00 5.9 GX 5-1 270.287 -25.084 1.5 5.074 -1.023 6.3 0.33 19.1 0.0 0.00 0.0 H 1820-303 275.921 -30.358 1.8 2.792 -7.914 7.8 0.51 15.1 0.0 0.00 0.0 GX 349+2 256.430 -36.450 2.0 349.080 +2.736 6.7 0.48 13.8 0.0 0.00 0.0 4U 1722-30 261.861 -30.798 2.6 356.311 +2.320 3.2 0.31 10.4 0.9 0.26 3.5 GX 3+1 266.993 -26.540 3.1 2.319 +0.799 2.5 0.30 8.3 0.0 0.00 0.0 3A 1822-371 276.383 -37.082 2.7 356.850 -11.236 6.4 0.64 9.9 0.0 0.00 0.0 XTE J1709-267 257.468 -26.680 4.0 357.501 +7.831 2.8 0.44 6.3 0.0 0.00 0.0 GRS 1741.9-2853 266.295 -28.965 3.6 359.925 +0.067 2.0 0.29 7.1 0.0 0.00 0.0 GX 9+1 270.450 -20.551 4.2 9.088 +1.089 2.9 0.49 5.9 0.0 0.00 0.0 GX 354-0 262.956 -33.826 4.0 354.295 -0.122 2.2 0.35 6.2 0.0 0.00 0.0 4U 1700-377 255.905 -37.899 4.2 347.671 +2.191 3.4 0.58 6.0 0.0 0.00 0.0 SLX 1735-269 264.565 -27.057 4.8 0.740 +2.371 1.4 0.28 5.2 0.0 0.00 0.0 IGR J17488-3253 267.286 -32.810 0.0 357.075 -2.652 1.7 0.00 5.5 0.0 0.00 0.0 IGR J17088-4008 257.261 -40.081 4.7 346.564 +0.036 3.5 0.65 5.3 0.0 0.00 0.0 IGR J18193-2542 274.884 -25.664 5.2 6.565 -4.944 2.3 0.48 4.8 0.0 0.00 0.0 IGR J17379-3747 264.578 -37.829 6.7 351.634 -3.391 1.7 0.47 3.6 0.0 0.00 0.0 IGR J17098-3628 257.494 -36.539 5.8 349.520 +1.997 2.1 0.49 4.2 0.0 0.00 0.0 1E 1743.1-2843 266.636 -28.713 0.0 0.295 -0.057 1.1 0.00 4.0 0.0 0.00 0.0 IGR J17464-2811 266.901 -28.250 7.2 0.813 -0.016 1.1 0.32 3.3 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 7.2 0.99 1.3 0.65 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.9 0.37 1.5 0.25 1A 1742-294 266.523 -29.515 359.559 -0.389 2.0 0.37 1.0 0.24 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.41 0.5 0.28 GX 3+1 266.983 -26.564 2.294 +0.794 34.2 0.61 4.1 0.32 GX 5-1 270.284 -25.079 5.077 -1.019 85.3 3.77 7.8 1.74
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