INTEGRAL Galactic Bulge Monitoring Revolution 0853: Observation start 2009-10-07T20:29 = MJD 55111.854
Total Observation GTI = 11123 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 1700-377 255.989 -37.845 0.5 347.754 +2.171 48.5 0.65 74.8 10.7 0.52 20.8 1E 1740.7-2942 265.980 -29.744 0.9 359.118 -0.107 12.7 0.34 36.9 7.5 0.30 24.7 GX 5-1 270.285 -25.092 1.1 5.066 -1.026 11.2 0.39 28.7 0.0 0.00 0.0 GRS 1758-258 270.303 -25.741 1.2 4.510 -1.361 10.0 0.41 24.4 5.3 0.34 15.6 GX 1+4 263.025 -24.734 1.4 1.955 +4.789 7.0 0.35 20.0 0.0 0.00 0.0 Ginga 1826-24 277.360 -23.802 1.6 9.265 -6.084 12.7 0.73 17.2 4.1 0.58 7.1 IGR J17252-3616 261.288 -36.267 2.5 351.506 -0.339 4.8 0.44 10.9 0.0 0.00 0.0 OAO 1657-415 255.254 -41.676 3.0 344.377 +0.277 10.5 1.21 8.7 0.0 0.00 0.0 H 1820-303 275.910 -30.362 2.3 2.784 -7.907 5.6 0.48 11.7 0.0 0.00 0.0 SLX 1744-299_300 266.883 -30.041 2.5 359.272 -0.929 3.4 0.32 10.6 0.0 0.00 0.0 4U 1722-30 261.878 -30.825 2.7 356.296 +2.293 3.7 0.39 9.6 0.0 0.00 0.0 IGR J17586-2129 269.641 -21.415 3.7 7.963 +1.316 3.6 0.52 6.9 0.0 0.00 0.0 3A 1822-371 276.369 -37.102 3.7 356.826 -11.235 4.6 0.66 7.0 0.0 0.00 0.0 GX 349+2 256.451 -36.397 3.5 349.132 +2.754 4.4 0.60 7.4 0.0 0.00 0.0 XTE J1751-305 267.872 -30.665 5.1 359.174 -1.982 1.8 0.36 4.8 1.4 0.31 4.6 GX 9+1 270.294 -20.476 4.6 9.081 +1.253 3.0 0.55 5.5 0.0 0.00 0.0 GRS 1741.9-2853 266.213 -28.932 4.1 359.916 +0.145 2.0 0.32 6.1 0.0 0.00 0.0 1A 1743-288 266.677 -28.819 3.9 0.223 -0.142 2.1 0.32 6.6 0.0 0.00 0.0 GX 3+1 267.053 -26.541 4.1 2.345 +0.752 2.2 0.36 6.2 0.0 0.00 0.0 3A 1728-169 262.899 -17.066 4.9 8.405 +9.011 5.0 0.97 5.1 0.0 0.00 0.0 IGR J17475-2822 266.943 -28.430 0.0 0.677 -0.141 1.5 0.00 4.2 0.0 0.00 0.0 NEW_1 267.865 -44.681 3.6 346.994 -9.028 12.9 1.84 7.0 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 in the 3-10 keV image > 5σ 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).NOTE: 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 5.0 0.44 0.6 0.28 1A 1742-294 266.523 -29.515 359.559 -0.389 6.1 0.43 0.9 0.31 GX 3+1 266.983 -26.564 2.294 +0.794 28.0 0.89 2.5 0.47 GX 5-1 270.284 -25.079 5.077 -1.019 88.4 5.40 6.7 2.33
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