INTEGRAL Galactic Bulge Monitoring Revolution 0369: Observation start 2005-10-23 = MJD 53666
Total Observation GTI = 11883 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRS 1758-258 270.304 -25.742 0.7 4.510 -1.362 16.2 0.32 50.9 11.2 0.26 43.0 Ginga 1826-24 277.377 -23.790 0.9 9.283 -6.092 17.5 0.50 34.8 7.2 0.37 19.3 1E 1740.7-2942 265.981 -29.748 1.1 359.115 -0.109 7.5 0.26 29.1 4.3 0.22 19.7 GX 1+4 263.010 -24.736 1.0 1.946 +4.800 9.7 0.32 30.2 0.0 0.00 0.0 H 1820-303 275.911 -30.359 1.4 2.787 -7.906 8.3 0.38 21.6 0.0 0.00 0.0 GX 349+2 256.466 -36.424 2.0 349.118 +2.728 7.8 0.56 14.0 0.0 0.00 0.0 4U 1700-377 256.000 -37.844 2.2 347.761 +2.165 7.8 0.62 12.6 0.0 0.00 0.0 4U 1722-30 261.886 -30.787 2.3 356.332 +2.308 3.5 0.30 11.7 1.3 0.23 5.6 3A 1822-371 276.422 -37.074 2.5 356.871 -11.260 5.7 0.53 10.7 0.0 0.00 0.0 GX 9+1 270.390 -20.467 2.6 9.133 +1.180 4.4 0.44 10.0 0.0 0.00 0.0 GX 354-0 262.992 -33.810 2.7 354.324 -0.139 3.4 0.35 9.7 0.0 0.00 0.0 GX 5-1 270.234 -25.089 2.8 5.046 -0.984 2.9 0.31 9.3 0.0 0.00 0.0 SLX 1744-299_300 266.869 -29.943 3.2 359.350 -0.869 2.1 0.26 8.0 0.0 0.00 0.0 SLX 1735-269 264.558 -27.025 3.5 0.763 +2.393 2.0 0.27 7.3 1.1 0.22 4.9 GX 3+1 267.005 -26.575 3.6 2.294 +0.771 2.1 0.30 7.1 0.0 0.00 0.0 1E 1743.1-2843 266.617 -28.794 4.3 0.218 -0.085 1.6 0.28 5.8 0.9 0.23 4.1 Oph Cluster 258.097 -23.331 4.4 0.595 +9.306 2.2 0.39 5.7 0.0 0.00 0.0 H 1702-429 256.540 -43.098 4.9 343.826 -1.342 10.3 2.07 5.0 0.0 0.00 0.0 1A 1742-294 266.631 -29.448 6.6 359.666 -0.434 1.2 0.32 3.6 0.0 0.00 0.0 XTE J1739-285 264.982 -28.517 5.1 359.700 +1.282 1.4 0.29 4.9 0.0 0.00 0.0 GX 13+1 273.623 -17.188 0.0 13.486 +0.099 3.4 0.00 4.4 0.0 0.00 0.0 GRS 1734-292 264.336 -29.123 5.2 358.885 +1.437 1.4 0.29 4.8 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 > 10σ 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).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; 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 1.39 2.6 0.90 1A 1742-294 266.523 -29.515 359.559 -0.389 5.3 0.43 1.3 0.24 GX 3+1 266.983 -26.564 2.294 +0.794 18.9 0.92 1.8 0.46 GX 5-1 270.284 -25.079 5.077 -1.019 101.1 2.75 7.5 1.11
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