INTEGRAL Galactic Bulge Monitoring Revolution 0492: Observation start 2006-10-23 = MJD 54031
Total Observation GTI = 12277 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+4 263.013 -24.742 0.6 1.942 +4.794 21.6 0.34 63.2 0.0 0.00 0.0 GX 5-1 270.290 -25.082 0.7 5.077 -1.024 16.6 0.33 50.4 1.5 0.27 5.6 4U 1700-377 255.992 -37.850 0.7 347.753 +2.167 34.9 0.71 49.0 10.2 0.56 18.4 GRS 1758-258 270.293 -25.744 1.1 4.503 -1.354 9.9 0.35 28.4 5.7 0.29 20.0 H 1820-303 275.932 -30.367 1.1 2.788 -7.926 12.1 0.43 28.3 0.0 0.00 0.0 1E 1740.7-2942 265.974 -29.755 1.2 359.106 -0.107 7.1 0.28 25.2 3.8 0.24 15.9 Ginga 1826-24 277.365 -23.795 1.3 9.273 -6.085 12.3 0.53 23.1 3.0 0.42 7.2 IGR J17497-2821 267.385 -28.344 1.7 0.952 -0.430 4.9 0.29 16.5 3.6 0.25 14.4 GX 349+2 256.436 -36.424 1.9 349.103 +2.748 8.7 0.60 14.5 0.0 0.00 0.0 4U 1722-30 261.905 -30.800 2.2 356.329 +2.288 3.9 0.31 12.4 1.8 0.25 7.3 GX 354-0 262.982 -33.818 2.1 354.313 -0.136 5.0 0.38 13.3 0.0 0.00 0.0 GX 9+1 270.397 -20.512 2.4 9.097 +1.152 4.8 0.43 11.2 0.0 0.00 0.0 3A 1822-371 276.425 -37.126 2.6 356.824 -11.285 6.0 0.59 10.2 0.0 0.00 0.0 1A 1742-294 266.497 -29.501 0.0 359.559 -0.362 2.7 0.00 8.6 0.0 0.00 0.0 GX 3+1 267.013 -26.565 3.0 2.306 +0.770 2.9 0.33 8.8 0.0 0.00 0.0 SLX 1744-299_300 266.862 -30.004 4.0 359.294 -0.895 1.8 0.29 6.3 1.1 0.24 4.6 H 1702-429 256.524 -43.084 4.1 343.831 -1.324 15.3 2.46 6.2 7.0 1.74 4.0 SLX 1735-269 264.644 -26.952 4.6 0.866 +2.368 1.6 0.29 5.4 1.4 0.23 6.0 IGR J17200-3116 260.025 -31.332 4.8 354.982 +3.320 1.8 0.34 5.2 0.0 0.00 0.0 1E 1743.1-2843 266.496 -28.760 0.0 0.192 +0.023 1.4 0.00 4.9 0.0 0.00 0.0 XB 1832-330 278.953 -32.970 5.2 1.558 -11.378 2.7 0.58 4.7 0.0 0.00 0.0 GRS 1741.9-2853 266.120 -28.925 0.0 359.880 +0.219 1.2 0.00 4.6 0.0 0.00 0.0 V2400 Oph 258.165 -24.267 0.0 359.856 +8.717 1.8 0.00 4.2 0.0 0.00 0.0 IGR J17088-4008 257.358 -40.177 0.0 346.532 -0.081 3.2 0.00 3.9 0.0 0.00 0.0 Swift J174535.5-2901 266.496 -29.090 0.0 359.911 -0.148 1.0 0.00 3.7 0.0 0.00 0.0 3A 1728-169 262.904 -16.917 6.3 8.536 +9.086 2.7 0.69 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 with 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 12.8 1.28 2.7 0.85 GX 3+1 266.983 -26.564 2.294 +0.794 21.7 0.55 3.1 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 115.0 2.26 19.8 1.09
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