INTEGRAL Galactic Bulge Monitoring Revolution 0724: Observation start 2008-09-18T07:55 = MJD 54727.331
Total Observation GTI = 12363 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 354-0 262.982 -33.834 0.6 354.299 -0.145 20.2 0.34 60.0 6.7 0.29 23.3 GRS 1758-258 270.311 -25.748 1.1 4.507 -1.371 9.3 0.32 29.0 6.7 0.27 24.6 Ginga 1826-24 277.363 -23.808 1.0 9.261 -6.089 17.4 0.58 30.1 7.5 0.46 16.3 1E 1740.7-2942 265.970 -29.751 1.1 359.107 -0.103 8.3 0.28 29.3 6.0 0.25 24.4 GX 1+4 263.015 -24.762 1.1 1.926 +4.781 8.3 0.31 26.8 0.0 0.00 0.0 GX 349+2 256.427 -36.420 1.4 349.102 +2.756 11.5 0.54 21.1 0.0 0.00 0.0 H 1820-303 275.921 -30.361 1.5 2.789 -7.915 8.6 0.43 19.8 0.0 0.00 0.0 OAO 1657-415 255.207 -41.653 1.9 344.373 +0.319 21.1 1.41 15.0 0.0 0.00 0.0 4U 1722-30 261.887 -30.797 2.3 356.324 +2.302 4.1 0.36 11.5 2.1 0.30 7.0 GX 5-1 270.275 -25.090 2.5 5.064 -1.017 3.3 0.32 10.5 0.0 0.00 0.0 3A 1822-371 276.450 -37.114 2.3 356.844 -11.298 6.8 0.57 11.9 0.0 0.00 0.0 GX 9+1 270.392 -20.557 3.2 9.056 +1.134 3.6 0.46 7.9 0.0 0.00 0.0 GX 3+1 266.972 -26.568 3.2 2.285 +0.800 2.6 0.33 8.0 0.0 0.00 0.0 MXB 1730-335 263.340 -33.395 3.8 354.830 -0.155 2.1 0.32 6.7 1.6 0.00 5.9 H 1702-429 256.596 -43.123 3.9 343.832 -1.389 14.1 2.15 6.5 6.1 0.00 3.8 3A 1728-169 262.889 -17.053 5.7 8.411 +9.026 3.0 0.69 4.3 0.0 0.00 0.0 1E 1742.9-2849 266.557 -28.809 6.2 0.178 -0.047 1.1 0.27 3.9 0.0 0.00 0.0 1A 1742-294 266.469 -29.477 6.1 359.567 -0.329 1.1 0.28 4.0 0.0 0.00 0.0 SLX 1744-299_300 266.870 -30.067 0.0 359.243 -0.933 1.2 0.00 3.9 0.0 0.00 0.0 SAX J1750.8-2900 267.491 -28.988 7.1 0.447 -0.840 1.0 0.29 3.4 1.4 0.25 5.7 SLX 1735-269 264.615 -26.932 7.4 0.870 +2.400 1.1 0.35 3.2 1.2 0.00 4.1 XTE J1751-305 267.923 -30.553 6.6 359.294 -1.962 1.2 0.00 3.7 0.0 0.00 0.0 GX 13+1 273.620 -17.263 6.6 13.419 +0.065 2.9 0.00 3.7 0.0 0.00 0.0 XTE J1710-281 257.479 -28.214 6.8 356.252 +6.926 1.4 0.00 3.5 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 7.4 1.32 3.0 0.97 MXB 1730-335 263.350 -33.388 354.841 -0.158 9.2 1.09 2.0 0.87 1A 1742-294 266.523 -29.515 359.559 -0.389 4.7 0.40 1.1 0.27 IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.1 0.48 0.0 0.00 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.6 0.42 0.8 0.32 GX 3+1 266.983 -26.564 2.294 +0.794 44.3 0.68 5.9 0.34 GX 5-1 270.284 -25.079 5.077 -1.019 102.4 2.51 10.0 1.09
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