INTEGRAL Galactic Bulge Monitoring Revolution 0426: Observation start 2006-04-09 = MJD 53834
Total Observation GTI = 7983 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== 4U 1700-377 255.985 -37.839 0.5 347.758 +2.178 51.7 0.73 70.6 12.1 0.58 21.0 GX 1+4 263.007 -24.740 0.9 1.941 +4.799 12.3 0.34 35.9 0.0 0.00 0.0 GRS 1758-258 270.320 -25.751 1.2 4.509 -1.380 10.8 0.42 25.6 7.8 0.35 22.4 Ginga 1826-24 277.372 -23.795 1.2 9.276 -6.090 17.8 0.69 26.0 6.5 0.55 11.9 H 1820-303 275.895 -30.347 2.2 2.791 -7.889 7.0 0.56 12.5 0.0 0.00 0.0 GX 349+2 256.435 -36.408 2.3 349.116 +2.758 6.8 0.59 11.4 0.0 0.00 0.0 GX 354-0 262.956 -33.819 3.1 354.300 -0.119 3.8 0.45 8.5 0.0 0.00 0.0 GX 3+1 266.956 -26.593 2.8 2.256 +0.799 3.2 0.33 9.5 0.0 0.00 0.0 GX 9+1 270.436 -20.512 3.3 9.115 +1.120 3.7 0.48 7.7 0.0 0.00 0.0 4U 1722-30 261.862 -30.806 3.0 356.304 +2.315 3.0 0.35 8.7 1.1 0.29 3.8 3A 1822-371 276.531 -37.088 2.9 356.896 -11.345 6.4 0.72 9.0 0.0 0.00 0.0 GX 5-1 270.308 -25.086 2.9 5.082 -1.041 3.3 0.36 9.1 0.0 0.00 0.0 IGR J17419-2802 265.422 -28.139 4.4 0.226 +1.153 2.0 0.36 5.7 0.0 0.00 0.0 SLX 1735-269 264.588 -27.013 3.4 0.788 +2.378 2.6 0.35 7.5 0.0 0.00 0.0 GX 13+1 273.584 -17.174 3.1 13.480 +0.138 7.3 0.87 8.3 0.0 0.00 0.0 GX 17+2 274.018 -14.030 3.3 16.443 +1.270 19.0 2.41 7.9 0.0 0.00 0.0 1A 1742-294 266.616 -29.536 0.0 359.583 -0.469 1.6 0.00 4.6 1.1 0.00 3.6 IGR J17252-3616 261.302 -36.302 0.0 351.484 -0.368 2.4 0.00 4.5 0.0 0.00 0.0 3A 1728-169 262.906 -16.911 5.4 8.542 +9.087 3.1 0.70 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1743-288 266.761 -28.883 0.207 -0.238 6.8 0.36 0.8 0.21 GX 354-0 262.989 -33.835 354.302 -0.150 16.7 1.51 4.8 1.00 1A 1742-294 266.523 -29.515 359.559 -0.389 3.0 0.35 0.8 0.22 GX 3+1 266.983 -26.564 2.294 +0.794 24.6 0.56 3.8 0.28 GX 5-1 270.284 -25.079 5.077 -1.019 88.9 2.19 6.1 0.91 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.5 0.38 0.5 0.24
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