INTEGRAL Galactic Bulge Monitoring Revolution 0366: Observation start 2005-10-12 = MJD 53655
Total Observation GTI = 12405 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 -37.851 0.5 347.748 +2.170 53.1 0.60 88.1 15.6 0.47 33.3 GX 5-1 270.285 -25.087 0.6 5.071 -1.023 18.4 0.28 65.4 0.0 0.00 0.0 GRS 1758-258 270.300 -25.739 0.8 4.511 -1.357 14.0 0.32 44.5 9.9 0.26 38.4 Ginga 1826-24 277.365 -23.795 0.9 9.273 -6.085 18.4 0.51 36.1 7.5 0.40 18.7 1E 1740.7-2942 265.984 -29.736 1.1 359.126 -0.105 7.4 0.28 26.6 4.7 0.23 19.9 GX 1+4 263.017 -24.751 1.1 1.936 +4.786 7.7 0.29 26.7 0.0 0.00 0.0 GX 349+2 256.443 -36.421 1.6 349.109 +2.745 8.7 0.49 17.8 0.0 0.00 0.0 H 1820-303 275.887 -30.372 1.7 2.766 -7.894 6.5 0.39 16.8 0.0 0.00 0.0 1A 1743-288 266.687 -28.867 2.2 0.188 -0.175 3.1 0.25 12.2 1.7 0.22 7.9 4U 1722-30 261.900 -30.776 2.3 356.347 +2.305 3.5 0.31 11.5 0.0 0.00 0.0 GX 354-0 263.004 -33.810 2.2 354.329 -0.147 3.6 0.29 12.2 0.0 0.00 0.0 3A 1822-371 276.467 -37.114 2.5 356.850 -11.311 5.7 0.55 10.4 0.0 0.00 0.0 GX 9+1 270.380 -20.559 3.1 9.049 +1.143 3.4 0.40 8.4 0.0 0.00 0.0 GX 3+1 267.003 -26.549 2.5 2.315 +0.786 2.8 0.26 10.7 0.0 0.00 0.0 SLX 1735-269 264.564 -27.017 3.3 0.774 +2.393 2.3 0.30 7.8 0.0 0.00 0.0 XTE J1739-285 265.067 -28.577 4.8 359.689 +1.187 1.4 0.26 5.2 0.0 0.00 0.0 GX 17+2 273.985 -14.033 4.0 16.426 +1.297 15.3 2.40 6.4 0.0 0.00 0.0 IGR J18027-2016 270.614 -20.228 4.5 9.445 +1.115 2.2 0.39 5.6 0.0 0.00 0.0 GX 13+1 273.629 -17.269 5.6 13.418 +0.055 3.0 0.00 4.4 0.0 0.00 0.0 H 1705-440 257.137 -44.192 6.1 343.210 -2.344 17.9 4.52 4.0 0.0 0.00 0.0 1A 1742-294 266.496 -29.501 0.0 359.559 -0.362 1.1 0.00 3.9 0.0 0.00 0.0 GRS 1741.9-2853 266.307 -28.925 0.0 359.965 +0.079 0.9 0.00 3.8 0.0 0.00 0.0 SLX 1744-299_300 266.876 -29.994 0.0 359.309 -0.900 1.0 0.00 3.7 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 1.8 0.34 0.7 0.20 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.2 0.43 1.1 0.22 GX 354-0 262.989 -33.835 354.302 -0.150 14.3 1.43 3.6 0.90 1A 1742-294 266.523 -29.515 359.559 -0.389 3.7 0.31 0.8 0.17 GX 3+1 266.983 -26.564 2.294 +0.794 20.6 0.52 2.8 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 95.4 2.08 18.9 1.06 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.0 0.31 0.4 0.18
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