INTEGRAL Galactic Bulge Monitoring Revolution 0672: Observation start 2008-04-14T09:48 = MJD 54570.409
Total Observation GTI = 9715 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17473-2721 266.827 -27.343 0.4 1.554 +0.510 49.8 0.39 129.4 20.8 0.30 68.3 GRO J1750-27 267.289 -26.644 0.9 2.366 +0.518 15.1 0.41 36.7 0.0 0.00 0.0 Ginga 1826-24 277.364 -23.798 1.2 9.270 -6.086 17.8 0.68 26.0 7.7 0.51 15.0 4U 1722-30 261.883 -30.791 1.3 356.326 +2.308 9.4 0.44 21.7 4.3 0.33 13.1 SAX J1750.8-2900 267.593 -29.032 1.4 0.455 -0.940 8.4 0.42 20.0 3.3 0.34 9.7 GRS 1758-258 270.313 -25.724 1.8 4.530 -1.361 6.4 0.40 15.9 4.7 0.31 15.0 H 1820-303 275.912 -30.372 1.7 2.776 -7.913 9.4 0.57 16.4 0.0 0.00 0.0 XTE J1810-189 272.588 -19.054 1.9 11.376 +0.065 10.0 0.69 14.5 4.3 0.52 8.3 1E 1740.7-2942 265.973 -29.745 2.3 359.114 -0.101 4.5 0.39 11.5 2.6 0.32 8.2 OAO 1657-415 255.183 -41.632 2.5 344.379 +0.346 23.0 2.12 10.8 0.0 0.00 0.0 GX 354-0 262.998 -33.827 2.4 354.313 -0.152 5.1 0.46 11.2 0.0 0.00 0.0 GX 3+1 266.918 -26.532 2.7 2.290 +0.860 4.0 0.00 9.6 0.0 0.00 0.0 GX 349+2 256.436 -36.442 3.1 349.089 +2.736 7.2 0.84 8.5 0.0 0.00 0.0 3A 1822-371 276.464 -37.138 3.4 356.827 -11.319 6.1 0.82 7.5 0.0 0.00 0.0 GX 9+1 270.377 -20.512 3.9 9.088 +1.168 3.8 0.59 6.5 0.0 0.00 0.0 GX 17+2 273.948 -13.998 3.5 16.439 +1.345 15.5 2.11 7.4 0.0 0.00 0.0 SLX 1744-299_300 266.868 -29.971 3.6 359.325 -0.882 2.9 0.42 7.0 0.0 0.00 0.0 GX 1+4 262.996 -24.698 4.9 1.971 +4.831 2.2 0.44 5.1 0.0 0.00 0.0 SLX 1735-269 264.612 -27.015 4.9 0.798 +2.359 2.0 0.00 5.0 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 3.6 0.61 1.1 0.46 IGR J17473-2721 266.825 -27.344 1.553 +0.510 9.2 0.56 6.1 0.37 GX 3+1 266.983 -26.564 2.294 +0.794 22.9 0.62 3.9 0.35 GX 5-1 270.284 -25.079 5.077 -1.019 52.3 1.64 4.8 0.81 GRO J1750-27 267.303 -26.643 2.373 +0.508 2.3 0.53 3.1 0.36
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