INTEGRAL Galactic Bulge Monitoring Revolution 0417: Observation start 2006-03-15 = MJD 53809
Total Observation GTI = 12318 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 5-1 270.282 -25.083 0.6 5.073 -1.019 16.2 0.29 55.9 0.9 0.24 3.6 GX 1+4 263.010 -24.753 0.8 1.932 +4.790 11.7 0.29 40.1 0.0 0.00 0.0 GRS 1758-258 270.293 -25.746 0.9 4.501 -1.356 10.9 0.29 37.0 7.2 0.24 29.9 Ginga 1826-24 277.357 -23.796 1.0 9.269 -6.079 17.5 0.53 33.1 6.8 0.41 16.5 1A 1742-294 266.517 -29.508 1.3 359.563 -0.381 6.0 0.26 23.0 2.4 0.22 10.7 GX 354-0 262.992 -33.835 1.5 354.303 -0.152 6.4 0.33 19.1 0.0 0.00 0.0 H 1820-303 275.921 -30.348 1.7 2.801 -7.909 7.1 0.42 17.0 1.1 0.33 3.3 XTE J1817-330 274.447 -33.009 1.8 359.832 -8.003 5.7 0.38 15.0 2.9 0.30 9.8 GX 349+2 256.417 -36.429 1.9 349.090 +2.756 7.2 0.51 14.3 0.0 0.00 0.0 3A 1822-371 276.444 -37.113 2.5 356.843 -11.293 5.7 0.53 10.6 0.0 0.00 0.0 GX 9+1 270.392 -20.544 2.7 9.067 +1.140 4.2 0.44 9.6 0.0 0.00 0.0 GX 3+1 266.999 -26.573 2.7 2.293 +0.777 3.0 0.30 9.9 0.0 0.00 0.0 GX 17+2 274.026 -14.045 2.8 16.434 +1.256 19.7 2.09 9.4 0.0 0.00 0.0 4U 1722-30 261.880 -30.833 3.5 356.290 +2.287 2.3 0.32 7.3 1.2 0.26 4.6 GX 13+1 273.589 -17.141 3.8 13.511 +0.149 4.9 0.74 6.6 0.0 0.00 0.0 SLX 1744-299_300 266.905 -29.975 3.6 359.338 -0.912 2.0 0.29 7.0 0.0 0.00 0.0 XTE J1739-285 264.972 -28.446 3.4 359.756 +1.327 2.0 0.27 7.5 1.2 0.22 5.5 SLX 1735-269 264.563 -26.990 3.3 0.796 +2.408 2.5 0.33 7.8 0.0 0.00 0.0 1A 1743-288 266.682 -28.924 0.0 0.136 -0.201 1.6 0.00 6.3 1.0 0.00 4.4 OAO 1657-415 255.136 -41.642 5.6 344.349 +0.368 6.1 1.39 4.4 0.0 0.00 0.0 3A 1728-169 262.883 -16.950 5.7 8.497 +9.085 2.9 0.66 4.3 0.0 0.00 0.0 Swift J174535.5-2901 266.306 -29.007 0.0 359.895 +0.037 1.0 0.00 4.2 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 > 10σ 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).NOTES: Fluxes for light curves are extracted from the images using
mosaic_spec
; 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 18.2 1.46 4.1 0.90 GX 3+1 266.983 -26.564 2.294 +0.794 29.4 0.54 4.2 0.29 GX 5-1 270.284 -25.079 5.077 -1.019 87.3 2.05 16.0 0.99
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