INTEGRAL Galactic Bulge Monitoring Revolution 0534: Observation start 2007-02-26 = MJD 54157
Total Observation GTI = 12314 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 1+4 263.011 -24.751 0.6 1.933 +4.790 21.1 0.33 63.3 0.0 0.00 0.0 GX 5-1 270.294 -25.087 0.8 5.075 -1.030 12.9 0.31 41.9 0.0 0.00 0.0 GRS 1758-258 270.290 -25.751 0.9 4.496 -1.356 11.5 0.30 37.6 8.0 0.25 32.1 1E 1740.7-2942 265.970 -29.746 0.9 359.112 -0.100 10.4 0.28 37.3 7.6 0.24 32.1 Ginga 1826-24 277.378 -23.805 1.0 9.270 -6.099 16.5 0.56 29.4 6.5 0.44 14.7 GX 349+2 256.439 -36.427 1.1 349.102 +2.744 15.0 0.51 29.2 0.0 0.00 0.0 H 1820-303 275.913 -30.361 1.6 2.786 -7.909 8.2 0.46 17.8 0.0 0.00 0.0 3A 1822-371 276.457 -37.104 2.1 356.855 -11.299 8.9 0.70 12.7 0.0 0.00 0.0 4U 1722-30 261.896 -30.786 2.9 356.336 +2.301 2.9 0.31 9.2 1.7 0.26 6.4 GX 354-0 262.997 -33.849 2.2 354.293 -0.164 4.3 0.35 12.2 0.0 0.00 0.0 1E 1742.8-2853 266.408 -28.922 3.3 0.014 +0.006 2.1 0.27 7.9 0.0 0.00 0.0 GX 3+1 266.989 -26.546 2.7 2.312 +0.798 2.7 0.28 9.6 0.0 0.00 0.0 SLX 1744-299_300 266.884 -30.038 3.3 359.275 -0.929 2.2 0.28 7.8 1.2 0.23 5.0 GRS 1734-292 264.307 -29.177 4.0 358.826 +1.429 1.8 0.29 6.3 0.0 0.00 0.0 GX 9+1 270.389 -20.541 3.4 9.068 +1.144 3.1 0.42 7.5 0.0 0.00 0.0 GX 13+1 273.666 -17.123 4.6 13.563 +0.094 4.1 0.75 5.5 0.0 0.00 0.0 3A 1728-169 262.853 -16.950 4.8 8.481 +9.109 3.5 0.69 5.1 0.0 0.00 0.0 SLX 1735-269 264.520 -27.078 5.4 0.700 +2.394 1.3 0.30 4.5 0.0 0.00 0.0 IGR J18027-1455 270.629 -14.843 6.3 14.145 +3.752 4.2 1.10 3.8 0.0 0.00 0.0 H 1705-440 257.277 -44.003 6.4 343.422 -2.312 14.6 0.00 3.8 0.0 0.00 0.0 SLX 1737-282 265.179 -28.348 0.0 359.935 +1.225 1.1 0.00 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 with 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 12.4 1.37 3.1 1.04 1A 1742-294 266.523 -29.515 359.559 -0.389 1.8 0.34 0.5 0.23 GX 3+1 266.983 -26.564 2.294 +0.794 27.2 0.56 3.4 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 102.2 2.49 13.4 1.10
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