INTEGRAL Galactic Bulge Monitoring Revolution 0778: Observation start 2009-02-25T13:20 = MJD 54887.556
Total Observation GTI = 10920 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 354-0 263.001 -33.829 0.8 354.312 -0.155 17.4 0.39 44.6 4.7 0.33 14.3 1E 1740.7-2942 265.984 -29.743 0.9 359.120 -0.109 11.5 0.31 37.5 8.4 0.27 31.6 Ginga 1826-24 277.377 -23.803 1.2 9.271 -6.098 14.2 0.56 25.3 5.7 0.46 12.6 GX 5-1 270.295 -25.087 1.5 5.076 -1.031 8.2 0.42 19.7 0.0 0.00 0.0 H 1820-303 275.929 -30.360 1.8 2.794 -7.921 7.3 0.47 15.6 0.0 0.00 0.0 GRS 1758-258 270.290 -25.758 1.8 4.490 -1.359 6.4 0.40 15.9 3.7 0.34 10.8 GX 349+2 256.442 -36.434 1.7 349.098 +2.738 10.4 0.61 16.9 0.0 0.00 0.0 GX 1+4 263.005 -24.773 2.5 1.912 +4.783 4.3 0.41 10.5 0.0 0.00 0.0 SLX 1735-269 264.534 -26.997 3.0 0.776 +2.426 3.0 0.35 8.6 0.0 0.00 0.0 3A 1822-371 276.452 -37.119 2.8 356.840 -11.302 5.5 0.59 9.3 0.0 0.00 0.0 4U 1722-30 261.890 -30.804 3.0 356.319 +2.295 3.3 0.38 8.7 1.5 0.32 4.6 GX 3+1 266.905 -26.537 3.6 2.280 +0.867 2.5 0.35 7.1 0.0 0.00 0.0 GX 13+1 273.674 -17.176 3.5 13.520 +0.062 6.7 0.90 7.4 0.0 0.00 0.0 SLX 1744-299_300 266.878 -29.999 0.0 359.305 -0.904 2.0 0.00 6.4 0.0 0.00 0.0 1A 1742-294 266.501 -29.505 0.0 359.558 -0.368 2.0 0.00 6.3 1.1 0.00 3.9 GX 9+1 270.374 -20.475 3.7 9.119 +1.189 3.4 0.50 6.8 0.0 0.00 0.0 XB 1832-330 278.809 -33.020 4.1 1.460 -11.290 3.6 0.59 6.1 0.0 0.00 0.0 IGR J17252-3616 261.221 -36.284 5.3 351.461 -0.304 2.1 0.46 4.7 0.0 0.00 0.0 GX 17+2 274.044 -13.975 5.1 16.503 +1.274 12.7 2.63 4.8 0.0 0.00 0.0 1E 1742.8-2853 266.560 -28.948 5.4 0.061 -0.122 1.5 0.33 4.6 0.0 0.00 0.0 SAX J1750.8-2900 267.580 -29.014 5.4 0.464 -0.921 1.4 0.32 4.5 0.0 0.00 0.0 IGR J18135-1751 273.380 -17.786 5.5 12.850 +0.017 3.6 0.81 4.4 0.0 0.00 0.0 GRS 1734-292 264.386 -29.151 6.0 358.885 +1.386 1.3 0.32 4.0 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== GX 354-0 262.989 -33.835 354.302 -0.150 8.6 1.70 2.4 1.09 GX 3+1 266.983 -26.564 2.294 +0.794 33.2 0.73 4.8 0.38 GX 5-1 270.284 -25.079 5.077 -1.019 96.6 2.18 12.9 0.99
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