INTEGRAL Galactic Bulge Monitoring Revolution 0293: Observation start 2005-03-08 = MJD 53437
Total Observation GTI = 8855 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 1700-377 255.982 -37.843 0.5 347.753 +2.177 46.1 0.65 71.4 10.8 0.50 21.5 1E 1740.7-2942 265.971 -29.756 0.9 359.103 -0.106 10.2 0.30 33.7 6.9 0.25 27.4 GRO J1655-40 253.500 -39.845 1.0 344.982 +2.457 38.4 1.19 32.2 29.2 0.90 32.4 GRS 1758-258 270.301 -25.755 0.9 4.498 -1.366 11.7 0.35 33.8 7.4 0.28 26.3 Ginga 1826-24 277.382 -23.801 1.2 9.274 -6.101 15.4 0.61 25.1 5.6 0.47 11.9 GX 349+2 256.414 -36.422 1.5 349.094 +2.763 10.5 0.56 18.8 0.0 0.00 0.0 GX 1+4 263.000 -24.745 1.6 1.933 +4.802 5.7 0.32 18.1 0.0 0.00 0.0 GX 354-0 262.976 -33.839 1.7 354.293 -0.144 6.0 0.35 16.8 0.0 0.00 0.0 1A 1742-294 266.542 -29.498 1.9 359.582 -0.395 4.7 0.31 14.9 1.6 0.00 6.2 GX 9+1 270.378 -20.532 2.2 9.071 +1.158 5.3 0.43 12.1 0.0 0.00 0.0 GX 5-1 270.299 -25.048 2.2 5.111 -1.015 4.0 0.33 12.1 0.0 0.00 0.0 H 1820-303 275.915 -30.372 2.3 2.777 -7.915 5.4 0.46 11.7 0.0 0.00 0.0 4U 1722-30 261.871 -30.862 2.7 356.262 +2.277 3.3 0.34 9.8 1.3 0.28 4.6 SLX 1735-269 264.582 -26.999 3.2 0.797 +2.390 2.8 0.34 8.2 1.6 0.29 5.5 GX 3+1 267.004 -26.534 3.6 2.328 +0.793 2.6 0.36 7.1 0.0 0.00 0.0 3A 1822-371 276.454 -37.109 3.3 356.850 -11.299 5.8 0.75 7.7 0.0 0.00 0.0 GX 17+2 273.994 -14.015 4.9 16.446 +1.298 10.7 2.10 5.1 0.0 0.00 0.0 3A 1728-169 262.952 -16.948 4.5 8.534 +9.031 3.8 0.68 5.5 0.0 0.00 0.0 SLX 1744-299_300 266.843 -30.079 0.0 359.221 -0.920 1.5 0.00 4.7 0.0 0.00 0.0 IGR J17252-3616 261.203 -36.287 5.3 351.451 -0.293 2.2 0.48 4.6 0.0 0.00 0.0 IGR J17456-2901 266.455 -29.013 0.0 359.957 -0.078 1.3 0.00 4.1 0.0 0.00 0.0 IGR J17407-2808 265.227 -28.159 5.3 0.118 +1.288 1.5 0.31 4.7 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 20.5 2.07 4.6 1.30 GX 3+1 266.983 -26.564 2.294 +0.794 25.4 0.57 4.0 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 95.5 2.20 9.8 0.91 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.3 0.50 0.4 0.27
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