INTEGRAL Galactic Bulge Monitoring Revolution 0477: Observation start 2006-09-09 = MJD 53987
Total Observation GTI = 12226 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+4 263.014 -24.747 0.6 1.938 +4.791 19.2 0.34 55.8 0.0 0.00 0.0 GX 5-1 270.285 -25.079 0.9 5.078 -1.019 12.7 0.34 37.5 0.0 0.00 0.0 GX 349+2 256.444 -36.422 1.0 349.109 +2.743 17.2 0.56 30.7 0.0 0.00 0.0 1A 1742-294 266.518 -29.510 1.1 359.561 -0.383 7.0 0.26 26.7 2.6 0.22 11.9 Ginga 1826-24 277.374 -23.808 1.1 9.265 -6.098 15.0 0.56 26.7 5.2 0.44 12.0 1E 1740.7-2942 265.975 -29.748 1.3 359.112 -0.104 6.1 0.26 22.9 3.4 0.22 15.2 GRS 1758-258 270.317 -25.740 1.4 4.518 -1.371 7.0 0.32 21.6 4.6 0.27 17.5 H 1820-303 275.929 -30.372 1.4 2.782 -7.926 8.2 0.41 20.0 0.0 0.00 0.0 GX 354-0 263.000 -33.837 1.4 354.305 -0.159 6.9 0.34 19.9 0.0 0.00 0.0 4U 1722-30 261.844 -30.807 2.4 356.294 +2.326 3.4 0.30 11.3 1.1 0.25 4.3 3A 1822-371 276.453 -37.094 2.6 356.863 -11.292 6.0 0.60 10.0 0.0 0.00 0.0 GX 3+1 267.034 -26.556 2.6 2.324 +0.759 2.8 0.28 10.0 0.0 0.00 0.0 SLX 1744-299_300 266.806 -30.030 3.1 359.247 -0.867 2.2 0.27 8.4 0.0 0.00 0.0 SLX 1735-269 264.562 -26.977 3.0 0.806 +2.416 2.4 0.28 8.7 1.4 0.23 6.1 GX 9+1 270.396 -20.570 3.7 9.046 +1.124 3.0 0.44 6.9 0.0 0.00 0.0 GX 17+2 273.967 -13.986 4.4 16.459 +1.335 10.5 1.85 5.7 0.0 0.00 0.0 1E 1743.1-2843 266.590 -28.761 0.0 0.234 -0.047 1.4 0.00 5.5 0.0 0.00 0.0 IGR J17252-3616 261.367 -36.322 4.4 351.496 -0.422 2.3 0.41 5.6 0.0 0.00 0.0 3A 1728-169 262.928 -16.959 4.6 8.512 +9.045 3.6 0.67 5.4 0.0 0.00 0.0 Swift J174535.5-2901 266.402 -29.090 0.0 359.867 -0.078 1.3 0.00 4.8 0.0 0.00 0.0 SLX 1737-282 265.147 -28.298 6.0 359.963 +1.275 1.1 0.26 4.0 0.0 0.00 0.0 H 1705-250 257.025 -25.071 5.6 358.585 +9.095 1.9 0.44 4.4 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 16.2 1.46 3.2 0.88 GX 3+1 266.983 -26.564 2.294 +0.794 25.2 0.58 3.5 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 112.4 2.33 16.8 1.10 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.33 0.6 0.25
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