INTEGRAL Galactic Bulge Monitoring Revolution 0550: Observation start 2007-04-15 = MJD 54205
Total Observation GTI = 11893 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 1+4 263.014 -24.742 0.8 1.942 +4.793 14.4 0.37 39.3 0.0 0.00 0.0 GRS 1758-258 270.307 -25.746 0.9 4.508 -1.367 12.2 0.33 37.1 8.9 0.26 33.8 Ginga 1826-24 277.368 -23.786 1.1 9.282 -6.083 16.6 0.57 29.0 6.9 0.43 16.0 1E 1740.7-2942 265.966 -29.741 1.3 359.114 -0.095 7.1 0.32 22.3 3.8 0.27 14.1 GX 354-0 262.979 -33.825 1.3 354.306 -0.137 8.0 0.37 22.0 0.0 0.00 0.0 1A 1742-294 266.530 -29.507 1.6 359.569 -0.390 5.7 0.31 18.3 2.3 0.26 9.0 H 1820-303 275.933 -30.367 1.7 2.789 -7.927 7.9 0.48 16.5 0.0 0.00 0.0 GX 349+2 256.425 -36.432 1.6 349.092 +2.750 11.2 0.65 17.3 0.0 0.00 0.0 4U 1722-30 261.885 -30.806 2.0 356.315 +2.299 4.6 0.34 13.4 1.6 0.27 5.8 3A 1822-371 276.423 -37.092 2.0 356.855 -11.269 9.3 0.69 13.4 0.0 0.00 0.0 GX 3+1 267.006 -26.565 2.1 2.303 +0.776 4.4 0.35 12.7 0.0 0.00 0.0 GX 17+2 274.001 -14.040 2.6 16.426 +1.280 17.2 1.71 10.1 0.0 0.00 0.0 GX 9+1 270.394 -20.513 2.5 9.095 +1.154 4.9 0.47 10.5 0.0 0.00 0.0 GX 5-1 270.284 -25.058 2.6 5.095 -1.008 3.6 0.36 10.0 0.0 0.00 0.0 OAO 1657-415 255.163 -41.607 3.6 344.389 +0.373 12.5 1.77 7.1 0.0 0.00 0.0 SLX 1744-299_300 266.828 -29.981 4.2 359.299 -0.858 2.0 0.33 6.0 0.0 0.00 0.0 SLX 1735-269 264.538 -27.012 4.9 0.766 +2.416 1.6 0.32 5.1 1.3 0.26 4.9 3A 1728-169 262.928 -17.001 5.1 8.476 +9.022 3.2 0.66 4.8 0.0 0.00 0.0 IGR J17195-4100 259.991 -40.942 0.0 347.078 -2.152 4.4 0.00 4.3 0.0 0.00 0.0 XB 1832-330 278.965 -32.917 6.2 1.611 -11.364 2.6 0.67 3.9 2.3 0.52 4.4 Swift J174535.5-2901 266.366 -29.001 0.0 359.927 -0.004 1.4 0.00 4.1 0.0 0.00 0.0 SLX 1737-282 265.275 -28.228 5.6 0.082 +1.217 1.4 0.31 4.4 0.0 0.00 0.0 IGR J17475-2822 266.834 -28.507 6.2 0.562 -0.099 1.2 0.00 3.9 0.0 0.00 0.0 Oph Cluster 258.117 -23.357 6.0 0.585 +9.276 1.8 0.46 4.0 0.0 0.00 0.0 IGR J18193-2542 274.830 -25.747 7.0 6.468 -4.939 1.5 0.45 3.5 0.0 0.00 0.0 IGR J17252-3616 261.359 -36.310 5.7 351.502 -0.411 2.0 0.46 4.3 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 3+1 266.983 -26.564 2.294 +0.794 32.5 0.57 4.4 0.27 GX 5-1 270.284 -25.079 5.077 -1.019 80.8 1.64 6.5 0.67
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