INTEGRAL Galactic Bulge Monitoring Revolution 0292: Observation start 2005-03-05 = MJD 53434
Total Observation GTI = 12329 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 1758-258 270.306 -25.740 0.8 4.512 -1.363 13.1 0.32 41.4 8.7 0.26 33.7 1E 1740.7-2942 265.977 -29.750 0.8 359.111 -0.107 10.0 0.25 40.6 6.9 0.21 33.3 Ginga 1826-24 277.357 -23.791 1.0 9.274 -6.076 16.2 0.52 31.2 5.8 0.41 14.3 GX 349+2 256.418 -36.421 1.1 349.096 +2.761 13.6 0.49 27.8 0.0 0.00 0.0 GX 5-1 270.275 -25.085 1.2 5.068 -1.014 7.9 0.33 23.8 0.0 0.00 0.0 GRO J1655-40 253.501 -39.850 1.3 344.979 +2.453 21.5 0.95 22.6 15.8 0.72 21.8 GX 1+4 262.998 -24.773 1.5 1.909 +4.789 6.6 0.34 19.6 0.0 0.00 0.0 GX 354-0 262.983 -33.836 1.4 354.298 -0.147 6.7 0.32 20.6 0.0 0.00 0.0 1A 1742-294 266.511 -29.518 1.5 359.551 -0.382 4.8 0.25 19.2 1.6 0.00 7.4 H 1820-303 275.908 -30.340 1.5 2.803 -7.895 7.3 0.40 18.5 0.0 0.00 0.0 4U 1700-377 255.971 -37.857 1.7 347.737 +2.176 8.9 0.54 16.5 0.0 0.00 0.0 4U 1722-30 261.893 -30.793 1.8 356.330 +2.300 4.5 0.28 15.7 1.7 0.23 7.2 OAO 1657-415 255.203 -41.657 1.9 344.368 +0.319 21.5 1.48 14.6 8.2 1.07 7.7 GX 9+1 270.369 -20.516 2.3 9.081 +1.173 4.5 0.39 11.5 0.0 0.00 0.0 SLX 1735-269 264.571 -26.981 2.2 0.807 +2.407 3.2 0.26 12.3 0.0 0.00 0.0 3A 1822-371 276.433 -37.109 2.4 356.843 -11.284 6.0 0.53 11.4 0.0 0.00 0.0 GX 3+1 267.033 -26.539 3.1 2.338 +0.768 2.3 0.28 8.3 0.0 0.00 0.0 GX 17+2 273.967 -14.092 3.7 16.366 +1.284 14.0 2.04 6.9 0.0 0.00 0.0 3A 1728-169 262.907 -16.966 3.4 8.496 +9.057 4.8 0.64 7.5 0.0 0.00 0.0 Oph Cluster 258.151 -23.380 5.4 0.584 +9.237 1.8 0.39 4.6 0.0 0.00 0.0 SLX 1744-299_300 266.941 -29.954 6.2 359.372 -0.927 1.0 0.26 3.9 0.0 0.00 0.0 1E 1743.1-2843 266.532 -28.748 6.5 0.219 +0.003 0.9 0.25 3.7 0.0 0.00 0.0 GX 13+1 273.590 -17.083 6.4 13.563 +0.176 2.7 0.71 3.8 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.34 1.4 0.21 GX 354-0 262.989 -33.835 354.302 -0.150 24.6 1.48 5.3 0.94 GX 3+1 266.983 -26.564 2.294 +0.794 26.6 0.54 4.0 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 86.4 2.15 7.6 0.91 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.6 0.36 0.7 0.23
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