INTEGRAL Galactic Bulge Monitoring Revolution 0720: Observation start 2008-09-05T00:02 = MJD 54714.002
Total Observation GTI = 12432 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 354-0 262.992 -33.837 0.7 354.302 -0.153 18.2 0.36 50.5 3.6 0.30 12.0 IGR J17473-2721 266.829 -27.349 0.8 1.550 +0.505 11.9 0.29 41.4 5.3 0.25 21.2 GX 5-1 270.293 -25.090 0.9 5.072 -1.030 11.8 0.32 37.5 0.0 0.00 0.0 GRS 1758-258 270.305 -25.746 0.9 4.507 -1.365 10.9 0.31 35.1 7.1 0.26 27.7 Ginga 1826-24 277.367 -23.795 1.1 9.274 -6.086 16.3 0.58 28.0 7.0 0.46 15.2 1E 1740.7-2942 265.992 -29.745 1.2 359.122 -0.115 7.2 0.29 24.8 4.3 0.25 17.6 GX 1+4 262.998 -24.748 1.8 1.930 +4.802 5.6 0.36 15.7 0.0 0.00 0.0 H 1820-303 275.918 -30.369 2.1 2.781 -7.916 6.4 0.48 13.2 0.0 0.00 0.0 4U 1722-30 261.907 -30.810 2.1 356.322 +2.281 4.4 0.33 13.3 1.6 0.27 6.1 OAO 1657-415 255.184 -41.658 2.0 344.358 +0.329 19.4 1.41 13.8 5.5 1.10 5.0 GX 3+1 266.969 -26.563 2.1 2.287 +0.805 3.9 0.30 13.0 0.0 0.00 0.0 GX 349+2 256.414 -36.429 2.2 349.089 +2.759 7.2 0.58 12.4 0.0 0.00 0.0 3A 1822-371 276.473 -37.042 2.9 356.918 -11.284 5.5 0.61 9.1 0.0 0.00 0.0 IGR J17379-3747 264.527 -37.747 3.2 351.683 -3.314 4.0 0.49 8.1 0.0 0.00 0.0 SLX 1735-269 264.581 -26.997 3.7 0.799 +2.391 2.2 0.31 6.9 0.0 0.00 0.0 GX 9+1 270.356 -20.499 3.6 9.090 +1.192 3.3 0.47 7.1 0.0 0.00 0.0 SLX 1744-299_300 266.826 -30.037 4.6 359.250 -0.885 1.5 0.29 5.4 0.0 0.00 0.0 H 1702-429 256.531 -43.057 4.8 343.855 -1.312 9.7 1.86 5.2 0.0 0.00 0.0 4U 1700-377 255.915 -37.774 5.0 347.776 +2.261 3.4 0.67 5.0 0.0 0.00 0.0 1E 1742.9-2849 266.498 -28.846 5.1 0.119 -0.023 1.4 0.28 4.9 0.0 0.00 0.0 GX 17+2 273.983 -14.078 0.0 16.385 +1.277 10.3 0.00 4.9 0.0 0.00 0.0 XTE J1810-189 272.546 -18.960 0.0 11.440 +0.145 2.7 0.00 4.7 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 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 11.2 1.43 3.7 1.05 1A 1742-294 266.523 -29.515 359.559 -0.389 3.5 0.39 0.8 0.23 IGR J17473-2721 266.825 -27.344 1.553 +0.510 3.1 0.49 1.8 0.30 GX 3+1 266.983 -26.564 2.294 +0.794 46.9 0.73 6.9 0.38 GX 5-1 270.284 -25.079 5.077 -1.019 121.9 2.73 17.9 1.24
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