INTEGRAL Galactic Bulge Monitoring Revolution 0368: Observation start 2005-10-19 = MJD 53662
Total Observation GTI = 13538 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 1700-377 255.995 -37.845 0.5 347.757 +2.168 51.4 0.64 80.6 14.3 0.49 29.0 GRS 1758-258 270.307 -25.744 0.7 4.509 -1.366 14.1 0.27 52.7 9.7 0.22 44.1 Ginga 1826-24 277.367 -23.790 0.8 9.278 -6.084 18.7 0.48 39.3 6.8 0.37 18.3 GX 5-1 270.287 -25.079 0.9 5.079 -1.021 10.0 0.29 34.1 0.0 0.00 0.0 GX 1+4 263.015 -24.744 0.9 1.942 +4.791 9.5 0.28 33.4 0.0 0.00 0.0 1E 1740.7-2942 265.979 -29.737 1.0 359.124 -0.102 7.6 0.25 30.1 4.5 0.21 21.0 GX 349+2 256.451 -36.414 1.3 349.118 +2.743 12.0 0.53 22.5 0.0 0.00 0.0 H 1820-303 275.910 -30.347 1.5 2.797 -7.901 6.8 0.35 19.3 0.0 0.00 0.0 XTE J1739-285 264.998 -28.463 2.3 359.753 +1.298 3.2 0.28 11.5 1.3 0.23 5.5 GX 354-0 262.997 -33.797 2.4 354.338 -0.135 3.3 0.30 11.2 0.0 0.00 0.0 4U 1722-30 261.898 -30.783 2.5 356.340 +2.301 3.0 0.28 10.8 1.2 0.22 5.6 OAO 1657-415 255.178 -41.666 2.7 344.349 +0.328 12.8 1.29 9.9 0.0 0.00 0.0 3A 1822-371 276.454 -37.137 2.5 356.824 -11.311 5.1 0.48 10.6 0.0 0.00 0.0 GX 3+1 266.995 -26.571 2.6 2.293 +0.781 2.8 0.27 10.2 0.0 0.00 0.0 GX 9+1 270.377 -20.617 2.9 8.997 +1.117 3.3 0.36 9.1 0.0 0.00 0.0 SLX 1735-269 264.604 -26.995 2.9 0.811 +2.376 2.5 0.27 9.1 1.2 0.23 5.4 GX 17+2 274.034 -14.013 3.7 16.465 +1.265 17.0 2.50 6.8 0.0 0.00 0.0 SLX 1744-299_300 266.813 -29.978 3.7 359.294 -0.845 1.7 0.25 6.9 0.9 0.21 4.1 1E 1742.8-2853 266.490 -28.935 3.9 0.039 -0.063 1.6 0.24 6.6 0.0 0.00 0.0 GRS 1734-292 264.354 -29.103 4.3 358.910 +1.435 1.6 0.27 5.9 0.0 0.00 0.0 IGR J17252-3616 261.281 -36.316 4.7 351.463 -0.362 2.0 0.38 5.3 0.0 0.00 0.0 H 1705-440 257.275 -44.203 6.0 343.260 -2.430 19.7 4.87 4.0 0.0 0.00 0.0 XB 1832-330 278.900 -32.971 4.7 1.537 -11.338 2.7 0.51 5.3 0.0 0.00 0.0 3A 1728-169 262.944 -16.918 5.7 8.556 +9.053 2.7 0.62 4.3 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 10.5 1.23 2.7 0.83 1A 1742-294 266.523 -29.515 359.559 -0.389 3.0 0.29 0.8 0.17 GX 3+1 266.983 -26.564 2.294 +0.794 21.6 0.52 3.0 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 110.0 2.24 14.6 1.03
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