INTEGRAL Galactic Bulge Monitoring Revolution 0365: Observation start 2005-10-10 = MJD 53653
Total Observation GTI = 13957 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 1700-377 255.986 -37.851 0.4 347.749 +2.169 66.8 0.56 120.3 20.1 0.42 47.9 GX 5-1 270.286 -25.080 0.5 5.077 -1.020 20.4 0.27 76.4 0.0 0.00 0.0 GRS 1758-258 270.306 -25.743 0.7 4.510 -1.364 14.1 0.30 46.9 10.2 0.24 41.9 Ginga 1826-24 277.378 -23.793 0.9 9.281 -6.094 16.8 0.45 37.2 7.7 0.35 22.2 GX 1+4 263.003 -24.744 1.0 1.936 +4.800 8.4 0.26 31.6 0.0 0.00 0.0 1E 1740.7-2942 265.989 -29.734 1.1 359.131 -0.108 7.4 0.27 27.5 4.9 0.23 21.4 H 1820-303 275.930 -30.358 1.5 2.796 -7.921 7.1 0.36 19.4 0.0 0.00 0.0 GX 349+2 256.456 -36.421 1.9 349.115 +2.737 6.9 0.49 14.1 0.0 0.00 0.0 GX 9+1 270.370 -20.545 2.1 9.056 +1.158 4.9 0.37 13.1 0.0 0.00 0.0 OAO 1657-415 255.189 -41.645 2.1 344.371 +0.335 18.7 1.46 12.7 0.0 0.00 0.0 4U 1722-30 261.891 -30.786 2.3 356.334 +2.305 3.5 0.30 11.8 1.2 0.24 4.9 1A 1743-288 266.731 -28.869 2.6 0.205 -0.209 2.4 0.24 10.3 1.3 0.20 6.7 GX 354-0 263.028 -33.823 2.6 354.330 -0.170 3.1 0.31 10.1 0.0 0.00 0.0 3A 1822-371 276.464 -37.102 2.4 356.860 -11.303 5.7 0.51 11.1 0.0 0.00 0.0 GX 3+1 266.963 -26.599 3.1 2.254 +0.790 2.1 0.25 8.5 0.0 0.00 0.0 SLX 1744-299_300 266.895 -30.040 3.1 359.278 -0.938 2.1 0.25 8.5 0.0 0.00 0.0 SLX 1735-269 264.579 -26.997 3.1 0.797 +2.393 2.3 0.28 8.4 1.2 0.23 5.1 GX 13+1 273.605 -17.193 3.9 13.473 +0.111 4.0 0.61 6.5 0.0 0.00 0.0 XTE J1739-285 265.034 -28.469 4.6 359.765 +1.269 1.4 0.25 5.5 0.0 0.00 0.0 NEW_0365 250.551 -34.402 4.2 347.663 +7.750 5.6 0.94 6.0 0.0 0.00 0.0 IGR J17597-2201 269.877 -21.997 4.3 7.567 +0.836 1.8 0.31 5.8 0.0 0.00 0.0 XB 1832-330 278.923 -33.038 4.5 1.484 -11.384 3.0 0.53 5.6 0.0 0.00 0.0 IGR J17354-3255 263.857 -33.007 5.6 355.391 -0.308 1.1 0.00 4.4 0.0 0.00 0.0 KS 1741-293 266.212 -29.254 0.0 359.641 -0.022 1.1 0.00 4.4 0.0 0.00 0.0 3A 1728-169 262.912 -16.962 6.1 8.501 +9.056 2.3 0.57 4.0 0.0 0.00 0.0 GRS 1734-292 264.445 -29.164 5.2 358.902 +1.334 1.2 0.25 4.7 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 14.1 1.38 4.1 0.92 1A 1742-294 266.523 -29.515 359.559 -0.389 3.9 0.29 0.7 0.18 GX 3+1 266.983 -26.564 2.294 +0.794 20.3 0.44 2.6 0.23 GX 5-1 270.284 -25.079 5.077 -1.019 95.0 1.73 22.9 0.94
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