INTEGRAL Galactic Bulge Monitoring Revolution 0412: Observation start 2006-02-27 = MJD 53793
Total Observation GTI = 12312 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 1700-377 255.985 -37.851 0.9 347.748 +2.171 23.9 0.64 37.1 6.7 0.51 13.2 GRS 1758-258 270.301 -25.734 0.9 4.516 -1.355 10.8 0.30 36.1 7.9 0.25 32.4 GX 5-1 270.284 -25.082 1.0 5.075 -1.020 9.9 0.31 31.8 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.798 1.0 9.273 -6.091 16.9 0.53 32.1 6.7 0.41 16.5 GX 1+4 263.016 -24.745 1.0 1.941 +4.790 11.2 0.36 31.5 0.0 0.00 0.0 1A 1742-294 266.515 -29.504 1.2 359.565 -0.378 6.0 0.25 23.8 1.7 0.21 8.1 GX 354-0 262.982 -33.811 1.5 354.318 -0.132 6.0 0.32 18.6 0.0 0.00 0.0 XTE J1817-330 274.433 -33.042 1.7 359.797 -8.008 6.2 0.38 16.4 3.4 0.30 11.4 H 1820-303 275.913 -30.357 1.7 2.790 -7.907 7.0 0.42 16.6 0.0 0.00 0.0 OAO 1657-415 255.188 -41.677 2.0 344.346 +0.315 15.3 1.14 13.3 0.0 0.00 0.0 GX 349+2 256.421 -36.411 2.0 349.106 +2.765 7.3 0.52 14.0 0.0 0.00 0.0 4U 1722-30 261.864 -30.795 2.6 356.314 +2.320 3.0 0.29 10.2 1.2 0.24 5.0 1A 1743-288 266.713 -28.857 3.1 0.207 -0.189 2.1 0.25 8.4 1.1 0.21 5.2 3A 1822-371 276.441 -37.121 3.0 356.835 -11.295 5.2 0.59 8.8 0.0 0.00 0.0 GX 3+1 266.943 -26.560 3.0 2.278 +0.826 2.3 0.26 8.8 0.0 0.00 0.0 GX 9+1 270.448 -20.492 3.8 9.138 +1.121 2.8 0.42 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.781 -29.994 0.0 359.266 -0.829 1.8 0.00 6.8 1.3 0.00 6.2 SLX 1735-269 264.567 -27.016 3.9 0.775 +2.392 1.7 0.26 6.4 0.8 0.22 3.7 GX 13+1 273.608 -17.118 4.3 13.540 +0.145 4.5 0.78 5.8 0.0 0.00 0.0 GX 17+2 273.929 -14.013 4.3 16.417 +1.354 11.5 1.95 5.9 0.0 0.00 0.0 Swift J174535.5-2901 266.306 -29.007 0.0 359.895 +0.037 1.2 0.00 4.9 0.0 0.00 0.0 3A 1728-169 262.873 -16.955 5.1 8.487 +9.091 3.0 0.63 4.8 0.0 0.00 0.0 IGR J17252-3616 261.347 -36.264 6.4 351.535 -0.377 1.5 0.00 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== XTE J1739-285 264.975 -28.496 359.714 +1.298 4.2 0.41 0.6 0.25 GX 354-0 262.989 -33.835 354.302 -0.150 20.2 1.51 4.0 0.89 1A 1742-294 266.523 -29.515 359.559 -0.389 1.9 0.37 1.2 0.23 GX 3+1 266.983 -26.564 2.294 +0.794 25.3 0.54 3.7 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 103.1 2.27 14.9 0.99
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