INTEGRAL Galactic Bulge Monitoring Revolution 0484: Observation start 2006-09-30 = MJD 54008
Total Observation GTI = 12413 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 1700-377 255.984 -37.851 0.5 347.748 +2.171 62.5 0.66 95.0 17.2 0.49 35.0 GX 5-1 270.287 -25.083 0.6 5.075 -1.023 19.8 0.31 63.6 1.2 0.25 5.0 GX 1+4 263.010 -24.745 0.7 1.938 +4.794 15.4 0.32 48.8 0.0 0.00 0.0 IGR J17497-2821 267.408 -28.360 0.8 0.948 -0.455 12.8 0.32 40.4 8.5 0.26 32.3 Ginga 1826-24 277.373 -23.801 1.0 9.271 -6.094 16.9 0.53 31.9 6.5 0.41 15.9 H 1820-303 275.925 -30.362 1.1 2.790 -7.918 13.2 0.46 28.7 0.0 0.00 0.0 1E 1740.7-2942 266.010 -29.749 1.3 359.127 -0.131 7.2 0.31 23.0 4.8 0.26 18.7 GRS 1758-258 270.306 -25.750 1.4 4.504 -1.368 7.2 0.34 21.4 5.2 0.27 19.2 GX 354-0 262.992 -33.836 1.4 354.303 -0.152 7.5 0.36 20.8 0.0 0.00 0.0 GX 349+2 256.410 -36.411 1.9 349.101 +2.772 8.1 0.55 14.7 0.0 0.00 0.0 4U 1722-30 261.891 -30.826 2.2 356.301 +2.283 3.8 0.30 12.6 1.7 0.24 7.0 1A 1742-294 266.506 -29.531 2.1 359.538 -0.385 3.7 0.29 12.7 1.2 0.00 4.8 3A 1822-371 276.428 -37.100 2.1 356.848 -11.276 7.4 0.58 12.6 0.0 0.00 0.0 GX 17+2 274.060 -14.055 3.3 16.440 +1.222 20.0 2.52 7.9 0.0 0.00 0.0 GX 3+1 267.000 -26.585 2.6 2.283 +0.770 3.0 0.29 10.2 0.0 0.00 0.0 GX 9+1 270.385 -20.525 3.5 9.080 +1.155 3.4 0.46 7.3 0.0 0.00 0.0 SLX 1735-269 264.564 -27.017 3.8 0.773 +2.394 2.0 0.29 6.7 1.0 0.00 4.1 IGR J18027-2016 270.701 -20.326 4.2 9.399 +0.995 2.8 0.47 6.0 0.0 0.00 0.0 1E 1742.9-2849 266.608 -28.824 4.8 0.189 -0.094 1.4 0.27 5.2 0.0 0.00 0.0 GRS 1734-292 264.314 -29.152 4.8 358.850 +1.437 1.5 0.28 5.2 1.4 0.23 5.9 3A 1728-169 262.873 -16.977 5.2 8.469 +9.079 3.1 0.66 4.8 0.0 0.00 0.0 XB 1832-330 278.925 -32.977 6.0 1.542 -11.360 2.4 0.59 4.1 0.0 0.00 0.0 IGR J17252-3616 261.231 -36.336 6.3 351.423 -0.339 1.6 0.42 3.9 0.0 0.00 0.0 SLX 1737-282 265.186 -28.343 6.5 359.942 +1.222 1.2 0.00 3.7 0.0 0.00 0.0 SLX 1744-299_300 266.877 -30.076 6.6 359.239 -0.943 1.2 0.00 3.7 0.0 0.00 0.0 IGR J17204-3554 260.190 -35.819 5.8 351.373 +0.647 1.8 0.43 4.2 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.2 0.37 1.1 0.25 GX 354-0 262.989 -33.835 354.302 -0.150 25.7 1.59 6.4 1.01 1A 1742-294 266.523 -29.515 359.559 -0.389 1.8 0.30 0.8 0.19 GX 3+1 266.983 -26.564 2.294 +0.794 30.3 0.55 4.2 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 98.1 2.11 22.8 1.13 IGR J17497-2821 267.404 -28.358 0.949 -0.451 2.4 0.38 1.3 0.22 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.0 0.33 0.6 0.23
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