INTEGRAL Galactic Bulge Monitoring Revolution 0663: Observation start 2008-03-18T18:01 = MJD 54543.751
Total Observation GTI = 12314 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.296 -26.645 0.5 2.369 +0.512 28.9 0.32 90.2 1.4 0.27 5.2 4U 1700-377 255.987 -37.836 0.8 347.761 +2.178 36.4 0.83 43.7 9.3 0.65 14.4 Ginga 1826-24 277.363 -23.803 0.9 9.265 -6.086 18.3 0.54 33.9 6.8 0.42 16.2 H 1820-303 275.922 -30.363 1.1 2.788 -7.917 12.8 0.45 28.4 0.0 0.00 0.0 4U 1722-30 261.874 -30.802 1.2 356.314 +2.308 8.3 0.34 24.1 2.3 0.28 8.3 GX 5-1 270.284 -25.090 1.4 5.067 -1.024 6.9 0.33 21.1 0.0 0.00 0.0 GX 354-0 262.973 -33.836 1.4 354.294 -0.139 8.3 0.40 20.7 1.9 0.33 5.9 GRS 1758-258 270.302 -25.748 1.8 4.504 -1.364 5.5 0.35 15.6 3.4 0.29 12.0 1E 1740.7-2942 265.977 -29.749 2.2 359.112 -0.107 4.3 0.34 12.5 1.8 0.29 6.4 GX 3+1 266.928 -26.585 0.0 2.250 +0.825 3.4 0.00 10.9 0.0 0.00 0.0 3A 1822-371 276.453 -37.142 2.7 356.819 -11.312 5.9 0.60 9.9 0.0 0.00 0.0 SAX J1750.8-2900 267.600 -29.043 2.6 0.448 -0.950 3.2 0.32 10.0 0.0 0.00 0.0 XTE J1810-189 272.579 -19.077 2.5 11.353 +0.061 5.7 0.54 10.7 3.5 0.43 8.3 GX 349+2 256.453 -36.410 3.0 349.123 +2.746 6.0 0.68 8.8 0.0 0.00 0.0 GX 9+1 270.364 -20.545 2.7 9.053 +1.163 3.7 0.39 9.6 0.0 0.00 0.0 GX 1+4 263.043 -24.749 3.3 1.951 +4.767 2.5 0.32 7.8 0.0 0.00 0.0 SLX 1735-269 264.574 -26.979 3.8 0.810 +2.406 2.2 0.32 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.845 -30.017 4.0 359.275 -0.888 2.1 0.33 6.3 0.0 0.00 0.0 MXB 1730-335 263.311 -33.379 4.4 354.830 -0.126 2.3 0.40 5.7 0.0 0.00 0.0 3A 1728-169 262.901 -16.943 4.4 8.512 +9.074 3.5 0.63 5.6 0.0 0.00 0.0 XB 1832-330 278.917 -33.051 4.4 1.470 -11.385 3.3 0.58 5.7 0.0 0.00 0.0 GX 17+2 273.966 -14.016 5.0 16.432 +1.321 7.8 1.57 5.0 0.0 0.00 0.0 1A 1742-294 266.514 -29.473 4.7 359.591 -0.361 1.7 0.32 5.3 0.0 0.00 0.0 IGR J17473-2721 266.834 -27.407 5.9 1.503 +0.471 1.2 0.00 4.1 0.0 0.00 0.0 V1223 Sgr 283.768 -31.215 7.4 4.912 -14.382 5.2 1.60 3.2 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 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 3+1 266.983 -26.564 2.294 +0.794 38.9 0.61 5.2 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 101.0 1.65 11.6 0.68 GRO J1750-27 267.303 -26.643 2.373 +0.508 6.6 0.50 6.5 0.30 SAX J1750.8-2900 267.603 -29.037 0.455 -0.949 11.0 0.52 2.3 0.28
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