INTEGRAL Galactic Bulge Monitoring Revolution 0849: Observation start 2009-09-27T13:13 = MJD 55101.551
Total Observation GTI = 12441 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 -37.848 0.6 347.752 +2.169 49.3 0.78 63.0 9.9 0.62 15.9 1E 1740.7-2942 265.977 -29.740 0.8 359.119 -0.102 12.7 0.30 41.9 7.6 0.27 28.4 GRS 1758-258 270.313 -25.731 1.0 4.524 -1.364 8.9 0.30 29.5 5.4 0.26 20.6 Ginga 1826-24 277.385 -23.793 1.1 9.283 -6.100 14.0 0.49 28.4 4.4 0.41 11.0 GX 1+4 262.989 -24.741 1.8 1.931 +4.812 5.2 0.33 15.7 0.0 0.00 0.0 OAO 1657-415 255.199 -41.640 2.0 344.380 +0.332 24.7 1.76 14.0 6.7 1.31 5.1 IGR J17511-3057 267.794 -30.967 2.3 358.881 -2.078 3.8 0.33 11.5 0.0 0.00 0.0 GX 5-1 270.288 -25.074 2.3 5.083 -1.019 3.8 0.32 11.8 0.0 0.00 0.0 4U 1722-30 261.888 -30.796 2.6 356.325 +2.302 4.1 0.40 10.2 1.4 0.33 4.4 IGR J17586-2129 269.674 -21.367 2.6 8.020 +1.314 4.1 0.40 10.1 1.2 0.00 3.6 GX 349+2 256.443 -36.364 2.5 349.154 +2.779 6.6 0.62 10.7 0.0 0.00 0.0 3A 1822-371 276.403 -37.075 3.3 356.863 -11.247 3.9 0.50 7.8 0.0 0.00 0.0 H 1820-303 275.889 -30.370 3.4 2.768 -7.895 3.1 0.41 7.6 0.0 0.00 0.0 SLX 1744-299_300 266.857 -30.015 4.0 359.283 -0.897 1.9 0.29 6.4 0.0 0.00 0.0 GX 3+1 267.019 -26.558 4.0 2.316 +0.769 1.9 0.30 6.4 0.0 0.00 0.0 SLX 1735-269 264.636 -26.995 4.1 0.826 +2.351 2.2 0.35 6.2 0.0 0.00 0.0 GX 9+1 270.427 -20.537 4.5 9.090 +1.115 2.6 0.47 5.6 0.0 0.00 0.0 GX 17+2 274.004 -14.015 4.8 16.450 +1.289 13.7 2.64 5.2 0.0 0.00 0.0 GRS 1747-312 267.670 -31.256 0.0 358.578 -2.135 1.5 0.00 4.7 0.0 0.00 0.0 XB 1832-330 279.024 -32.980 5.1 1.575 -11.436 2.4 0.51 4.8 0.0 0.00 0.0 IGR J17375-3022 264.389 -30.451 5.9 357.788 +0.686 1.4 0.35 4.1 0.0 0.00 0.0 1E 1742.9-2849 266.627 -28.873 5.7 0.156 -0.133 1.2 0.28 4.3 0.0 0.00 0.0 GX 354-0 263.036 -33.788 0.0 354.363 -0.158 1.3 0.00 3.8 0.0 0.00 0.0 IGR J17464-2811 266.926 -28.210 6.4 0.858 -0.014 1.1 0.00 3.8 0.0 0.00 0.0 1RXS J165424.7-29541 253.625 -29.910 6.0 352.838 +8.592 3.5 0.88 4.0 0.0 0.00 0.0 PSR J1649-4349 252.493 -43.879 6.7 341.390 +0.472 41.0 0.00 3.6 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 5.0 0.40 0.9 0.24 GX 3+1 266.983 -26.564 2.294 +0.794 25.2 0.64 3.3 0.34 GX 5-1 270.284 -25.079 5.077 -1.019 87.6 1.55 5.3 0.64
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