INTEGRAL Galactic Bulge Monitoring Revolution 0601: Observation start 2007-09-15 = MJD 54358
Total Observation GTI = 11364 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 1700-377 255.991 -37.848 0.5 347.754 +2.168 69.3 0.77 89.7 21.5 0.60 36.0 GX 5-1 270.285 -25.078 0.7 5.078 -1.018 17.8 0.35 51.5 0.0 0.00 0.0 GX 1+4 263.005 -24.743 0.8 1.938 +4.800 15.8 0.37 42.8 0.0 0.00 0.0 Ginga 1826-24 277.371 -23.810 1.0 9.263 -6.097 18.5 0.56 33.0 8.0 0.44 18.0 H 1820-303 275.916 -30.369 1.2 2.780 -7.915 11.3 0.43 26.1 0.0 0.00 0.0 SAX J1810.8-2609 272.690 -26.141 1.7 5.208 -3.430 6.6 0.40 16.6 3.7 0.32 11.5 GX 349+2 256.451 -36.424 1.7 349.111 +2.738 10.2 0.63 16.3 0.0 0.00 0.0 GRS 1758-258 270.282 -25.741 2.4 4.501 -1.345 4.0 0.35 11.4 2.7 0.29 9.2 4U 1722-30 261.905 -30.815 2.5 356.317 +2.279 3.9 0.37 10.5 1.9 0.31 6.1 GX 3+1 267.019 -26.559 2.3 2.315 +0.769 3.9 0.33 11.9 0.0 0.00 0.0 3A 1822-371 276.438 -37.058 3.4 356.891 -11.265 4.6 0.61 7.6 0.0 0.00 0.0 3A 1728-169 262.961 -16.973 4.1 8.517 +9.010 4.4 0.72 6.1 0.0 0.00 0.0 GX 9+1 270.452 -20.496 4.3 9.137 +1.116 2.7 0.46 5.8 0.0 0.00 0.0 SLX 1735-269 264.568 -26.955 3.5 0.827 +2.424 2.3 0.32 7.3 0.0 0.00 0.0 GX 354-0 262.980 -33.817 3.9 354.313 -0.134 2.2 0.34 6.4 0.0 0.00 0.0 SLX 1744-299_300 266.949 -30.045 4.2 359.298 -0.980 2.1 0.35 5.9 0.0 0.00 0.0 GX 17+2 274.048 -14.046 3.7 16.443 +1.237 14.2 2.05 7.0 0.0 0.00 0.0 H 1702-429 256.556 -43.046 4.5 343.875 -1.320 13.8 2.48 5.6 0.0 0.00 0.0 1E 1742.9-2849 266.606 -28.838 5.0 0.175 -0.099 1.5 0.30 4.9 0.0 0.00 0.0 GX 13+1 273.612 -17.150 4.2 13.514 +0.126 4.8 0.79 6.0 0.0 0.00 0.0 GRS 1734-292 264.475 -29.139 4.9 358.937 +1.325 1.6 0.32 5.1 0.0 0.00 0.0 1A 1742-294 266.508 -29.490 0.0 359.574 -0.365 1.4 0.00 4.5 0.0 0.00 0.0 SAX J1712.6-3739 258.223 -37.687 5.7 348.937 +0.850 2.3 0.00 4.3 0.0 0.00 0.0 1H 1746-370 267.433 -37.002 6.4 353.526 -4.897 1.7 0.00 3.8 0.0 0.00 0.0 IGR J16482-3036 252.173 -30.592 6.4 351.506 +9.144 3.1 0.00 3.8 0.0 0.00 0.0 IGR J17252-3616 261.322 -36.324 5.8 351.474 -0.394 1.9 0.46 4.2 0.0 0.00 0.0 IGR J16500-3307 252.479 -33.195 5.5 349.634 +7.296 3.2 0.71 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 > 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 8.6 1.35 1.9 0.99 1A 1742-294 266.523 -29.515 359.559 -0.389 3.5 0.35 0.8 0.21 GX 3+1 266.983 -26.564 2.294 +0.794 31.6 0.61 4.3 0.31 GX 5-1 270.284 -25.079 5.077 -1.019 94.8 2.28 17.6 1.10
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