INTEGRAL Galactic Bulge Monitoring Revolution 0353: Observation start 2005-09-03 = MJD 53616
Total Observation GTI = 12418 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 1700-377 255.984 -37.842 0.4 347.755 +2.177 75.8 0.62 122.5 22.8 0.47 48.5 GRS 1758-258 270.303 -25.741 0.8 4.510 -1.361 11.9 0.28 42.0 8.8 0.23 38.6 1E 1740.7-2942 265.979 -29.741 0.9 359.119 -0.104 8.7 0.25 34.6 5.1 0.21 24.5 Ginga 1826-24 277.373 -23.805 0.9 9.267 -6.096 17.4 0.51 33.8 7.2 0.40 18.2 GX 354-0 262.982 -33.833 1.2 354.300 -0.144 7.7 0.31 24.9 0.0 0.00 0.0 GX 1+4 263.010 -24.757 1.3 1.928 +4.788 7.2 0.32 22.8 0.0 0.00 0.0 KS 1741-293 266.212 -29.337 0.0 359.570 -0.065 4.6 0.00 18.7 2.2 0.00 10.5 GX 5-1 270.290 -25.086 1.7 5.074 -1.027 4.7 0.29 16.1 0.0 0.00 0.0 GX 349+2 256.411 -36.430 1.8 349.086 +2.760 8.0 0.52 15.3 0.0 0.00 0.0 GX 17+2 274.008 -14.023 1.8 16.445 +1.282 31.0 2.03 15.2 0.0 0.00 0.0 1A 1742-294 266.590 -29.501 0.0 359.601 -0.432 3.3 0.00 13.5 1.3 0.00 6.1 H 1820-303 275.934 -30.361 2.0 2.794 -7.925 5.4 0.41 13.4 0.0 0.00 0.0 4U 1722-30 261.882 -30.826 2.3 356.297 +2.289 3.5 0.29 11.9 1.0 0.23 4.5 SLX 1735-269 264.560 -27.024 2.3 0.766 +2.393 3.0 0.26 11.5 1.1 0.22 5.1 3A 1822-371 276.456 -37.137 2.5 356.825 -11.312 5.7 0.54 10.6 0.0 0.00 0.0 IGR J17464-3213 266.551 -32.244 2.3 357.240 -1.828 3.1 0.26 11.8 1.8 0.22 8.4 GX 3+1 267.051 -26.588 2.8 2.304 +0.729 2.4 0.25 9.5 0.0 0.00 0.0 SLX 1744-299_300 266.851 -30.019 3.8 359.277 -0.894 1.7 0.25 6.7 0.0 0.00 0.0 GX 9+1 270.373 -20.505 3.6 9.093 +1.175 2.8 0.39 7.2 0.0 0.00 0.0 XTE J1818-245 274.598 -24.553 3.6 7.428 -4.195 3.4 0.47 7.1 1.4 0.38 3.5 IGR J17456-2901 266.401 -29.008 0.0 359.937 -0.034 1.4 0.00 5.7 0.0 0.00 0.0 XTE J1739-285 265.008 -28.561 5.6 359.675 +1.239 1.1 0.25 4.4 0.0 0.00 0.0 IGR J17252-3616 261.336 -36.253 4.8 351.539 -0.363 2.0 0.38 5.2 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 2.1 0.33 0.4 0.21 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.3 0.36 1.3 0.23 GX 354-0 262.989 -33.835 354.302 -0.150 18.1 1.54 4.2 0.97 GX 3+1 266.983 -26.564 2.294 +0.794 18.9 0.51 2.5 0.26 GX 5-1 270.284 -25.079 5.077 -1.019 110.9 2.24 11.4 0.98 IGR J17464-3213 266.567 -32.229 357.260 -1.832 3.4 0.51 0.4 0.31
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