INTEGRAL Galactic Bulge Monitoring Revolution 0714: Observation start 2008-08-18T01:21 = MJD 54696.057
Total Observation GTI = 7162 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 5-1 270.283 -25.086 0.9 5.071 -1.021 18.1 0.48 37.5 0.0 0.00 0.0 4U 1700-377 255.988 -37.849 0.9 347.751 +2.170 39.5 1.05 37.5 8.9 0.81 11.1 IGR J17473-2721 266.835 -27.344 0.9 1.557 +0.503 13.2 0.36 36.8 5.0 0.32 15.7 GX 354-0 262.984 -33.826 1.0 354.308 -0.142 14.6 0.49 29.8 4.1 0.40 10.2 Ginga 1826-24 277.366 -23.799 1.3 9.269 -6.087 17.6 0.80 22.1 7.3 0.63 11.6 GRS 1758-258 270.308 -25.739 1.3 4.515 -1.363 9.7 0.45 21.7 6.1 0.37 16.5 GX 1+4 263.005 -24.739 1.5 1.941 +4.801 9.1 0.47 19.4 0.0 0.00 0.0 GX 349+2 256.436 -36.430 1.6 349.099 +2.744 17.2 0.95 18.1 0.0 0.00 0.0 1E 1740.7-2942 265.917 -29.736 1.9 359.096 -0.055 5.7 0.40 14.3 4.3 0.34 12.7 4U 1722-30 261.875 -30.788 2.1 356.325 +2.315 6.3 0.48 13.2 2.4 0.38 6.3 OAO 1657-415 255.226 -41.657 2.3 344.378 +0.305 22.4 1.93 11.6 0.0 0.00 0.0 H 1820-303 275.930 -30.353 2.6 2.800 -7.918 6.1 0.61 10.1 0.0 0.00 0.0 3A 1822-371 276.426 -37.092 2.7 356.856 -11.271 7.6 0.77 9.8 0.0 0.00 0.0 GX 3+1 266.972 -26.518 0.0 2.327 +0.826 3.4 0.00 8.5 0.0 0.00 0.0 GX 9+1 270.428 -20.484 3.5 9.136 +1.141 4.4 0.60 7.3 0.0 0.00 0.0 H 1702-429 256.689 -43.067 3.3 343.917 -1.410 17.8 2.28 7.8 0.0 0.00 0.0 1A 1742-294 266.570 -29.490 4.6 359.602 -0.411 2.1 0.39 5.4 0.0 0.00 0.0 SLX 1735-269 264.612 -27.097 5.0 0.728 +2.315 2.0 0.41 4.9 0.0 0.00 0.0 AX J1736.4-2910 264.185 -29.206 6.9 358.744 +1.504 1.6 0.46 3.5 0.0 0.00 0.0 IGR J17407-2808 265.193 -28.132 6.1 0.125 +1.329 1.8 0.44 4.0 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== IGR J17473-2721 266.825 -27.344 1.553 +0.510 4.0 0.62 2.1 0.36 GX 3+1 266.983 -26.564 2.294 +0.794 52.8 0.92 8.3 0.47 GX 5-1 270.284 -25.079 5.077 -1.019 87.7 2.38 18.2 1.21
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