INTEGRAL Galactic Bulge Monitoring Revolution 0845: Observation start 2009-09-15T03:17 = MJD 55089.137
Total Observation GTI = 14952 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 1E 1740.7-2942 265.972 -29.740 0.8 359.117 -0.099 11.6 0.26 44.5 7.9 0.23 34.7 GX 5-1 270.279 -25.087 0.9 5.068 -1.019 10.9 0.31 34.5 0.0 0.00 0.0 GRS 1758-258 270.306 -25.752 1.0 4.502 -1.368 10.1 0.32 32.0 6.7 0.27 24.9 Ginga 1826-24 277.363 -23.787 1.1 9.279 -6.079 13.6 0.51 26.9 5.5 0.40 13.7 GX 1+4 262.998 -24.752 1.1 1.926 +4.800 8.4 0.31 27.0 0.0 0.00 0.0 IGR J17511-3057 267.794 -30.959 1.3 358.888 -2.075 7.3 0.31 23.2 2.7 0.27 9.9 GX 349+2 256.437 -36.433 1.6 349.097 +2.741 9.5 0.55 17.3 0.0 0.00 0.0 IGR J17586-2129 269.676 -21.391 2.0 7.999 +1.300 5.7 0.41 14.0 0.0 0.00 0.0 H 1820-303 275.878 -30.359 2.0 2.774 -7.881 5.9 0.43 13.9 0.0 0.00 0.0 4U 1722-30 261.877 -30.805 2.2 356.311 +2.304 4.0 0.32 12.5 1.7 0.27 6.2 3A 1822-371 276.446 -37.109 2.4 356.847 -11.293 5.8 0.52 11.1 0.0 0.00 0.0 IGR J17252-3616 261.292 -36.284 3.7 351.493 -0.351 2.7 0.38 6.9 0.0 0.00 0.0 OAO 1657-415 255.224 -41.681 3.8 344.359 +0.292 7.0 1.06 6.6 0.0 0.00 0.0 GX 9+1 270.410 -20.511 4.3 9.104 +1.142 2.5 0.42 5.8 0.0 0.00 0.0 SLX 1735-269 264.539 -26.976 3.8 0.796 +2.434 2.0 0.30 6.7 1.3 0.26 4.9 GX 17+2 273.982 -14.038 5.0 16.420 +1.297 11.0 2.21 5.0 0.0 0.00 0.0 XB 1832-330 278.938 -32.988 5.7 1.536 -11.374 2.4 0.55 4.3 2.6 0.44 5.9 1E 1742.8-2853 266.465 -28.927 5.9 0.035 -0.040 1.0 0.25 4.1 0.0 0.00 0.0 SLX 1744-299_300 266.816 -29.983 5.5 359.291 -0.850 1.2 0.27 4.5 0.0 0.00 0.0 GX 354-0 262.945 -33.936 5.5 354.198 -0.175 1.3 0.28 4.5 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.9 0.35 1.3 0.22 1A 1742-294 266.523 -29.515 359.559 -0.389 5.2 0.32 0.9 0.20 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.1 0.33 0.7 0.23 GX 3+1 266.983 -26.564 2.294 +0.794 27.8 0.59 3.3 0.34 GX 5-1 270.284 -25.079 5.077 -1.019 120.4 2.51 15.8 1.14
Go back to Bulge home page