INTEGRAL Galactic Bulge Monitoring Revolution 0655: Observation start 2008-02-23 = MJD 54519
Total Observation GTI = 10570 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 J1750-27 267.301 -26.649 0.4 2.367 +0.507 42.0 0.35 118.4 1.9 0.29 6.5 GX 5-1 270.287 -25.088 0.8 5.071 -1.025 15.1 0.37 40.3 0.0 0.00 0.0 Ginga 1826-24 277.366 -23.806 1.0 9.263 -6.091 17.7 0.60 29.8 6.6 0.45 14.6 4U 1722-30 261.865 -30.802 1.1 356.308 +2.315 11.0 0.41 26.4 4.8 0.33 14.8 H 1820-303 275.915 -30.375 1.5 2.775 -7.916 9.3 0.47 19.6 0.0 0.00 0.0 OAO 1657-415 255.198 -41.662 1.8 344.362 +0.319 26.8 1.73 15.6 7.3 1.22 5.9 1A 1742-294 266.528 -29.527 1.9 359.552 -0.399 4.6 0.33 14.1 1.2 0.27 4.3 GX 3+1 266.954 -26.515 0.0 2.322 +0.841 4.1 0.00 12.0 0.0 0.00 0.0 GRS 1758-258 270.300 -25.733 2.2 4.516 -1.355 4.5 0.37 12.2 2.0 0.30 6.7 GX 349+2 256.408 -36.447 2.6 349.072 +2.752 7.9 0.78 10.2 0.0 0.00 0.0 3A 1822-371 276.445 -37.106 3.1 356.849 -11.291 4.6 0.56 8.2 0.0 0.00 0.0 IGR J17456-2901 266.460 -28.987 3.9 359.982 -0.067 2.2 0.34 6.4 0.0 0.00 0.0 GX 9+1 270.424 -20.568 3.3 9.061 +1.103 3.9 0.50 7.8 0.0 0.00 0.0 GX 1+4 263.088 -24.697 4.4 2.017 +4.761 2.4 0.42 5.7 0.0 0.00 0.0 IGR J17252-3616 261.314 -36.260 0.0 351.524 -0.352 2.8 0.00 5.6 0.0 0.00 0.0 GX 354-0 263.011 -33.824 4.2 354.321 -0.159 2.3 0.39 6.0 0.0 0.00 0.0 1E 1740.7-2942 265.950 -29.761 4.8 359.089 -0.093 1.7 0.33 5.1 1.7 0.27 6.3 IGR J18027-2016 270.726 -20.310 0.0 9.426 +0.984 2.4 0.00 4.8 0.0 0.00 0.0 SLX 1744-299_300 266.831 -29.968 0.0 359.311 -0.853 1.6 0.00 4.8 0.0 0.00 0.0 GX 13+1 273.659 -17.146 5.9 13.539 +0.088 3.8 0.00 4.2 0.0 0.00 0.0 MXB 1730-335 263.381 -33.293 5.0 354.934 -0.128 1.9 0.39 4.9 0.0 0.00 0.0 Oph Cluster 258.034 -23.430 0.0 0.480 +9.297 2.1 0.00 3.7 0.0 0.00 0.0 SLX 1735-269 264.583 -26.982 6.5 0.812 +2.398 1.3 0.36 3.7 1.3 0.29 4.4 3A 1728-169 262.893 -16.892 7.7 8.552 +9.109 3.0 0.96 3.1 0.0 0.00 0.0 AX J1700.2-4220 255.186 -42.411 0.0 343.766 -0.135 6.8 0.00 3.4 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.2 0.41 0.7 0.23 GX 3+1 266.983 -26.564 2.294 +0.794 34.4 0.84 5.5 0.47 SLX 1746-331 267.461 -33.199 356.816 -2.976 4.3 0.81 0.0 0.00 GX 5-1 270.284 -25.079 5.077 -1.019 77.5 2.03 13.3 1.02 GRO J1750-27 267.300 -26.647 2.368 +0.508 14.0 0.75 9.5 0.45
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