INTEGRAL Galactic Bulge Monitoring Revolution 0427: Observation start 2006-04-14 = MJD 53839
Total Observation GTI = 12326 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 5-1 270.286 -25.080 0.7 5.077 -1.021 17.1 0.32 53.5 0.0 0.00 0.0 GRS 1758-258 270.303 -25.737 0.9 4.514 -1.359 10.3 0.28 36.6 7.5 0.23 32.2 4U 1700-377 255.983 -37.838 0.9 347.758 +2.180 24.4 0.67 36.3 7.7 0.53 14.7 GX 1+4 263.011 -24.736 0.9 1.947 +4.798 10.5 0.30 35.5 0.0 0.00 0.0 H 1820-303 275.903 -30.357 0.9 2.786 -7.900 13.6 0.41 33.4 0.0 0.00 0.0 Ginga 1826-24 277.369 -23.787 1.0 9.282 -6.085 16.2 0.51 31.6 6.9 0.40 17.4 GX 349+2 256.419 -36.403 1.3 349.111 +2.771 11.6 0.52 22.4 0.0 0.00 0.0 GX 354-0 262.981 -33.818 1.4 354.313 -0.135 6.4 0.32 20.1 0.0 0.00 0.0 4U 1722-30 261.880 -30.791 2.3 356.325 +2.310 3.3 0.28 11.7 1.6 0.24 6.6 GX 3+1 267.016 -26.590 2.4 2.286 +0.755 3.0 0.27 10.9 0.0 0.00 0.0 3A 1822-371 276.444 -37.088 2.5 356.866 -11.283 5.6 0.53 10.5 0.0 0.00 0.0 GX 9+1 270.379 -20.502 3.2 9.098 +1.172 3.2 0.39 8.2 0.0 0.00 0.0 SLX 1735-269 264.562 -26.979 3.3 0.804 +2.415 2.2 0.28 7.8 0.0 0.00 0.0 SLX 1744-299_300 266.856 -30.021 3.7 359.277 -0.899 1.8 0.26 6.9 1.1 0.23 5.1 GX 17+2 274.022 -14.034 3.4 16.442 +1.265 19.0 2.50 7.6 0.0 0.00 0.0 IGR J17456-2901 266.400 -29.008 0.0 359.937 -0.034 1.5 0.00 6.0 0.0 0.00 0.0 KS 1741-293 266.306 -29.337 0.0 359.613 -0.135 1.7 0.00 5.9 0.0 0.00 0.0 Oph Cluster 258.077 -23.422 4.8 0.509 +9.269 2.2 0.42 5.2 0.0 0.00 0.0 MXB 1730-335 263.372 -33.316 4.4 354.911 -0.134 1.7 0.29 5.7 0.0 0.00 0.0 GX 13+1 273.618 -17.112 5.3 13.550 +0.139 3.4 0.00 4.7 0.0 0.00 0.0 GRS 1734-292 264.376 -29.143 5.0 358.887 +1.397 1.4 0.29 4.9 1.2 0.24 5.1 3A 1728-169 262.909 -16.969 5.3 8.494 +9.054 3.0 0.64 4.6 0.0 0.00 0.0 1A 1743-288 266.870 -28.842 0.0 0.292 -0.299 1.0 0.00 3.9 0.0 0.00 0.0 4U 1705-32 257.123 -32.281 6.6 352.769 +4.773 1.4 0.00 3.7 0.0 0.00 0.0 OAO 1657-415 255.189 -41.663 5.8 344.357 +0.324 6.2 1.47 4.2 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1743-288 266.761 -28.883 0.207 -0.238 7.9 0.38 0.9 0.21 GX 354-0 262.989 -33.835 354.302 -0.150 14.7 1.46 3.8 0.94 1A 1742-294 266.523 -29.515 359.559 -0.389 4.5 0.35 1.2 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 26.6 0.57 4.0 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 100.9 2.25 16.7 1.05
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