INTEGRAL Galactic Bulge Monitoring Revolution 0543: Observation start 2007-03-25 = MJD 54184
Total Observation GTI = 12136 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+4 263.009 -24.742 0.6 1.940 +4.797 22.8 0.33 68.7 0.0 0.00 0.0 GX 5-1 270.277 -25.077 0.6 5.076 -1.012 17.9 0.31 58.0 1.3 0.25 5.3 GRS 1758-258 270.305 -25.746 0.9 4.506 -1.365 12.1 0.32 38.1 8.9 0.26 34.5 Ginga 1826-24 277.361 -23.796 0.9 9.270 -6.082 18.6 0.56 33.4 7.0 0.43 16.4 1E 1740.7-2942 265.975 -29.737 1.0 359.121 -0.099 10.3 0.33 31.1 6.7 0.28 23.9 GX 354-0 262.990 -33.818 1.5 354.316 -0.142 7.1 0.38 18.6 0.0 0.00 0.0 1A 1742-294 266.504 -29.503 1.6 359.561 -0.369 5.7 0.32 18.0 1.8 0.00 6.7 H 1820-303 275.889 -30.366 1.8 2.772 -7.893 7.0 0.44 15.8 0.0 0.00 0.0 GX 3+1 266.978 -26.568 2.0 2.288 +0.795 4.5 0.33 13.8 0.0 0.00 0.0 GX 9+1 270.448 -20.483 2.2 9.146 +1.125 5.3 0.43 12.3 0.0 0.00 0.0 4U 1700-377 255.981 -37.830 2.1 347.763 +2.185 9.8 0.77 12.7 3.9 0.60 6.5 GRS 1741.9-2853 266.331 -28.898 2.8 359.999 +0.075 2.9 0.30 9.4 1.2 0.26 4.9 OAO 1657-415 255.180 -41.656 2.5 344.358 +0.333 24.0 2.26 10.6 6.4 1.70 3.8 3A 1822-371 276.447 -37.067 2.8 356.886 -11.276 5.7 0.61 9.4 0.0 0.00 0.0 4U 1722-30 261.894 -30.804 2.4 356.321 +2.292 4.0 0.37 11.0 2.0 0.29 6.9 GX 349+2 256.429 -36.388 2.8 349.128 +2.774 5.9 0.63 9.4 0.0 0.00 0.0 GX 13+1 273.628 -17.133 3.6 13.536 +0.120 4.7 0.66 7.1 0.0 0.00 0.0 IGR J18027-2016 270.681 -20.183 0.0 9.515 +1.083 2.8 0.00 6.4 0.0 0.00 0.0 GX 17+2 273.988 -14.026 3.6 16.432 +1.298 10.4 1.47 7.1 0.0 0.00 0.0 SLX 1735-269 264.529 -27.031 4.1 0.744 +2.412 2.0 0.33 6.2 2.1 0.28 7.5 SLX 1744-299_300 266.850 -29.987 4.1 359.304 -0.877 1.9 0.30 6.2 0.0 0.00 0.0 XB 1832-330 278.919 -33.000 4.5 1.518 -11.365 3.3 0.60 5.5 2.0 0.46 4.4 3A 1728-169 262.952 -16.951 4.7 8.532 +9.029 3.3 0.63 5.2 0.0 0.00 0.0 IGR J16500-3307 252.443 -33.178 0.0 349.628 +7.330 3.6 0.00 4.1 0.0 0.00 0.0 GRS 1734-292 264.330 -29.118 7.5 358.886 +1.444 1.1 0.33 3.2 0.0 0.00 0.0 AX J1749.1-2733 267.216 -27.578 0.0 1.532 +0.093 1.1 0.00 3.8 0.9 0.00 3.8 NEW_1 257.264 -31.092 3.9 353.802 +5.381 2.9 0.45 6.4 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 3+1 266.983 -26.564 2.294 +0.794 29.7 0.52 3.8 0.26 GX 5-1 270.284 -25.079 5.077 -1.019 77.0 1.34 15.4 0.66
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