INTEGRAL Galactic Bulge Monitoring Revolution 0658: Observation start 2008-03-03T12:56 = MJD 54528.539
Total Observation GTI = 11612 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1750-27 267.296 -26.644 0.4 2.369 +0.512 38.8 0.34 114.9 1.5 0.27 5.5 4U 1700-377 255.985 -37.846 0.5 347.752 +2.173 55.2 0.70 78.7 16.4 0.53 31.0 H 1820-303 275.921 -30.359 1.0 2.791 -7.914 16.1 0.52 31.3 0.0 0.00 0.0 Ginga 1826-24 277.362 -23.790 1.1 9.277 -6.080 18.5 0.65 28.7 6.4 0.49 13.0 4U 1722-30 261.881 -30.800 1.3 356.318 +2.304 8.3 0.36 23.1 3.9 0.29 13.5 GRS 1758-258 270.289 -25.760 2.1 4.487 -1.359 4.4 0.35 12.6 3.0 0.28 10.8 GX 349+2 256.409 -36.415 2.0 349.097 +2.770 8.2 0.61 13.4 0.0 0.00 0.0 GX 3+1 266.950 -26.548 0.0 2.292 +0.827 3.3 0.00 9.7 0.0 0.00 0.0 1E 1740.7-2942 265.977 -29.715 2.6 359.141 -0.089 3.2 0.31 10.2 1.7 0.26 6.6 3A 1822-371 276.484 -37.066 2.8 356.900 -11.302 5.9 0.62 9.5 0.0 0.00 0.0 OAO 1657-415 255.129 -41.619 2.7 344.364 +0.386 11.9 1.22 9.7 0.0 0.00 0.0 GX 9+1 270.361 -20.535 2.9 9.061 +1.170 4.7 0.52 8.9 0.0 0.00 0.0 GX 17+2 274.018 -13.995 3.5 16.474 +1.287 26.8 3.68 7.3 0.0 0.00 0.0 SLX 1735-269 264.554 -26.962 4.2 0.815 +2.430 2.0 0.34 6.0 0.0 0.00 0.0 3A 1728-169 262.968 -16.963 4.0 8.529 +9.009 6.2 0.98 6.3 0.0 0.00 0.0 GX 354-0 262.988 -33.836 3.8 354.300 -0.150 2.6 0.38 6.8 0.0 0.00 0.0 GX 5-1 270.291 -25.105 0.0 5.057 -1.036 2.0 0.00 5.6 0.0 0.00 0.0 GX 1+4 263.001 -24.687 4.9 1.982 +4.832 2.1 0.41 5.1 0.0 0.00 0.0 XB 1832-330 278.950 -32.995 5.0 1.533 -11.386 3.2 0.65 5.0 0.0 0.00 0.0 IGR J17464-2811 266.865 -28.109 6.3 0.917 +0.084 1.2 0.00 3.9 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 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 7.4 1.21 1.6 0.79 MXB 1730-335 263.350 -33.388 354.841 -0.158 7.7 0.96 1.8 0.71 GX 3+1 266.983 -26.564 2.294 +0.794 31.7 0.77 4.7 0.41 SLX 1746-331 267.461 -33.199 356.816 -2.976 4.3 0.85 1.7 1.12 GX 5-1 270.284 -25.079 5.077 -1.019 68.6 2.66 5.1 1.13 GRO J1750-27 267.300 -26.647 2.368 +0.508 14.3 0.76 10.5 0.44
Go back to Bulge home page