INTEGRAL Galactic Bulge Monitoring Revolution 0719: Observation start 2008-09-02T01:15 = MJD 54711.052
Total Observation GTI = 8754 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 1700-377 255.993 -37.850 0.5 347.753 +2.166 69.8 0.84 83.3 18.7 0.65 28.6 GX 354-0 262.989 -33.831 0.8 354.305 -0.148 19.7 0.46 43.1 5.0 0.38 13.3 IGR J17473-2721 266.823 -27.333 0.9 1.561 +0.518 13.1 0.36 36.0 5.8 0.31 18.4 GX 5-1 270.277 -25.077 1.1 5.076 -1.012 13.1 0.48 27.6 0.0 0.00 0.0 Ginga 1826-24 277.374 -23.793 1.2 9.278 -6.092 18.4 0.72 25.7 6.4 0.56 11.4 GRS 1758-258 270.309 -25.750 1.3 4.506 -1.370 9.9 0.45 21.9 7.7 0.37 20.8 1E 1740.7-2942 265.979 -29.737 1.4 359.123 -0.102 7.5 0.36 21.0 5.5 0.30 18.0 GX 349+2 256.438 -36.437 1.8 349.094 +2.738 11.1 0.71 15.7 0.0 0.00 0.0 GX 1+4 263.008 -24.736 2.0 1.945 +4.801 6.0 0.44 13.6 0.0 0.00 0.0 4U 1722-30 261.858 -30.785 2.1 356.319 +2.329 5.3 0.41 12.7 1.6 0.34 4.9 H 1820-303 275.913 -30.359 2.2 2.788 -7.908 6.9 0.57 12.1 0.0 0.00 0.0 GX 3+1 266.989 -26.559 2.7 2.301 +0.792 3.7 0.38 9.9 0.0 0.00 0.0 3A 1822-371 276.415 -37.153 3.2 356.795 -11.290 5.9 0.73 8.1 0.0 0.00 0.0 GX 9+1 270.354 -20.548 3.8 9.047 +1.169 3.8 0.55 6.8 0.0 0.00 0.0 SLX 1735-269 264.588 -26.964 3.5 0.830 +2.403 2.8 0.38 7.3 2.0 0.32 6.1 H 1702-429 256.527 -43.040 4.1 343.867 -1.299 12.7 2.06 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.852 -29.986 4.7 359.305 -0.878 1.9 0.37 5.3 0.0 0.00 0.0 GX 17+2 273.995 -14.019 4.5 16.442 +1.295 16.5 2.98 5.6 0.0 0.00 0.0 1E 1742.8-2853 266.519 -28.942 5.4 0.047 -0.088 1.6 0.36 4.5 0.0 0.00 0.0 IGR J17464-2811 266.794 -28.216 6.2 0.793 +0.083 1.4 0.36 3.9 0.0 0.00 0.0 3A 1728-169 262.968 -17.008 6.0 8.490 +8.986 3.5 0.86 4.1 0.0 0.00 0.0 4U 1705-32 257.103 -32.337 0.0 352.715 +4.753 2.2 0.00 4.0 0.0 0.00 0.0** NOTE **: ScWs 07190002-0003 were not included in analysis due to poor pointing data.
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 10.4 1.45 3.3 1.02 1A 1742-294 266.523 -29.515 359.559 -0.389 3.9 0.45 0.9 0.30 IGR J17473-2721 266.825 -27.344 1.553 +0.510 4.9 0.57 1.9 0.33 GX 3+1 266.983 -26.564 2.294 +0.794 52.0 0.86 6.9 0.44 GX 5-1 270.284 -25.079 5.077 -1.019 142.2 4.42 18.8 2.05
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