INTEGRAL Galactic Bulge Monitoring Revolution 0716: Observation start 2008-08-24T01:27 = MJD 54702.061
Total Observation GTI = 1648 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.990 -37.844 1.0 347.756 +2.172 65.7 2.02 32.5 13.5 1.60 8.5 IGR J17473-2721 266.832 -27.328 1.6 1.570 +0.514 15.0 0.87 17.2 5.0 0.77 6.5 GX 354-0 262.980 -33.832 1.6 354.301 -0.142 17.9 0.99 18.1 5.1 0.83 6.1 GX 5-1 270.296 -25.086 2.2 5.077 -1.031 12.1 1.00 12.1 0.0 0.00 0.0 GRS 1758-258 270.299 -25.728 2.9 4.520 -1.351 9.2 1.01 9.2 7.5 0.84 9.0 Ginga 1826-24 277.370 -23.815 2.8 9.258 -6.098 15.6 1.64 9.6 7.0 1.31 5.3 GX 1+4 263.038 -24.759 3.1 1.940 +4.765 8.5 1.00 8.5 0.0 0.00 0.0 1E 1740.7-2942 265.970 -29.724 3.2 359.130 -0.088 6.8 0.85 8.0 3.3 0.74 4.5 GX 17+2 274.013 -14.056 3.6 16.418 +1.262 35.0 4.89 7.2 0.0 0.00 0.0 IGR J17252-3616 261.223 -36.318 4.6 351.434 -0.324 6.8 1.25 5.4 0.0 0.00 0.0 4U 1722-30 261.841 -30.830 3.8 356.274 +2.316 6.9 1.04 6.6 3.5 0.84 4.1 H 1820-303 275.876 -30.387 4.1 2.749 -7.892 8.3 1.35 6.1 0.0 0.00 0.0 GX 349+2 256.453 -36.453 4.3 349.089 +2.719 9.6 1.63 5.9 0.0 0.00 0.0 GX 3+1 266.953 -26.589 4.8 2.258 +0.804 4.6 0.90 5.1 0.0 0.00 0.0 OAO 1657-415 255.184 -41.702 5.6 344.324 +0.303 16.8 0.00 4.4 0.0 0.00 0.0 H 1702-429 256.506 -43.064 0.0 343.839 -1.301 22.9 0.00 4.0 0.0 0.00 0.0 1A 1742-294 266.564 -29.561 6.6 359.539 -0.444 3.1 0.84 3.6 0.0 0.00 0.0** NOTE **: Due to an error in the instrument parameters at the beginning of the revolution, there is very high deadtime in the ISGRI data - hence the mosaic only has an effective time of 1600 seconds.
JEM-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 8.8 1.57 3.1 1.06 IGR J17473-2721 266.825 -27.344 1.553 +0.510 2.9 0.53 1.7 0.34 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.3 0.58 0.7 0.31 GX 3+1 266.983 -26.564 2.294 +0.794 52.2 0.89 7.3 0.45 GX 5-1 270.284 -25.079 5.077 -1.019 114.8 4.02 16.8 1.85
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