INTEGRAL Galactic Bulge Monitoring Revolution 0303: Observation start 2005-04-07 = MJD 53467
Total Observation GTI = 12318 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 1700-377 255.987 -37.849 0.4 347.750 +2.170 76.2 0.56 135.3 22.9 0.42 54.1 GRS 1758-258 270.305 -25.740 0.8 4.513 -1.362 13.7 0.33 42.2 9.4 0.26 36.0 GX 349+2 256.437 -36.415 1.0 349.111 +2.752 14.2 0.48 29.6 0.0 0.00 0.0 GX 1+4 263.009 -24.753 1.0 1.930 +4.791 9.3 0.29 32.5 0.0 0.00 0.0 Ginga 1826-24 277.359 -23.798 1.1 9.268 -6.082 14.5 0.50 28.9 5.3 0.39 13.4 1E 1740.7-2942 265.984 -29.741 1.2 359.122 -0.108 7.0 0.28 24.8 3.8 0.24 16.1 1A 1742-294 266.507 -29.507 1.6 359.559 -0.373 5.1 0.29 17.5 1.6 0.00 6.6 GX 354-0 262.983 -33.821 1.5 354.310 -0.138 5.7 0.31 18.5 1.0 0.00 4.1 H 1820-303 275.904 -30.370 1.7 2.775 -7.906 6.5 0.39 16.5 0.0 0.00 0.0 3A 1822-371 276.446 -37.121 2.0 356.836 -11.298 7.6 0.55 13.8 0.0 0.00 0.0 4U 1722-30 261.887 -30.826 2.3 356.300 +2.286 3.8 0.32 11.9 1.2 0.26 4.8 GX 9+1 270.365 -20.563 2.4 9.038 +1.152 4.5 0.41 10.9 0.0 0.00 0.0 SLX 1735-269 264.561 -26.966 2.4 0.815 +2.423 3.3 0.30 11.0 1.5 0.25 6.0 1E 1742.8-2853 266.400 -28.919 2.9 0.012 +0.013 2.2 0.24 9.0 0.0 0.00 0.0 GX 5-1 270.341 -25.123 3.4 5.065 -1.085 2.2 0.28 7.6 0.0 0.00 0.0 GX 3+1 266.976 -26.572 2.9 2.283 +0.795 2.4 0.27 9.1 0.0 0.00 0.0 3A 1728-169 262.964 -16.951 3.3 8.537 +9.020 4.8 0.61 7.9 0.0 0.00 0.0 GX 17+2 274.009 -14.012 4.1 16.455 +1.286 15.1 2.47 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.893 -29.978 4.6 359.331 -0.904 1.5 0.27 5.4 0.0 0.00 0.0 IGR J18027-2016 270.642 -20.218 0.0 9.466 +1.097 2.0 0.00 5.1 0.0 0.00 0.0 GX 13+1 273.560 -17.060 4.7 13.569 +0.212 3.9 0.72 5.3 0.0 0.00 0.0 XTE J1743-363 265.662 -36.321 5.4 353.375 -3.329 1.8 0.38 4.6 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 22.6 1.50 4.4 0.88 1A 1742-294 266.523 -29.515 359.559 -0.389 1.6 0.31 0.9 0.20 GX 3+1 266.983 -26.564 2.294 +0.794 23.8 0.50 3.6 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 92.0 2.09 6.1 0.90 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.0 0.37 0.9 0.22
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