INTEGRAL Galactic Bulge Monitoring Revolution 0600: Observation start 2007-09-12 = MJD 54355
Total Observation GTI = 11755 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 1700-377 255.986 -37.846 0.5 347.753 +2.173 50.4 0.68 74.4 15.7 0.53 29.5 GX 1+4 263.009 -24.748 0.9 1.935 +4.794 13.5 0.39 34.9 0.0 0.00 0.0 Ginga 1826-24 277.372 -23.793 1.0 9.278 -6.090 17.8 0.58 30.7 8.4 0.46 18.1 GX 5-1 270.272 -25.085 1.1 5.067 -1.012 10.1 0.38 26.9 0.0 0.00 0.0 H 1820-303 275.920 -30.357 1.3 2.792 -7.912 10.2 0.43 23.7 0.0 0.00 0.0 GX 354-0 262.976 -33.844 1.2 354.288 -0.146 8.6 0.36 23.9 2.2 0.30 7.5 GX 349+2 256.437 -36.416 1.6 349.110 +2.752 10.8 0.59 18.2 0.0 0.00 0.0 SAX J1810.8-2609 272.664 -26.178 1.8 5.164 -3.428 5.5 0.36 15.1 2.3 0.30 7.8 GRS 1758-258 270.306 -25.724 2.0 4.527 -1.354 5.1 0.38 13.5 2.9 0.32 9.0 3A 1822-371 276.467 -37.102 2.3 356.861 -11.305 7.5 0.64 11.7 0.0 0.00 0.0 GX 17+2 274.021 -14.030 2.7 16.445 +1.268 22.8 2.33 9.8 0.0 0.00 0.0 GX 9+1 270.451 -20.501 2.7 9.131 +1.114 4.4 0.45 9.8 0.0 0.00 0.0 4U 1722-30 261.923 -30.789 3.0 356.347 +2.280 3.1 0.35 8.8 2.0 0.29 6.8 GX 3+1 267.020 -26.588 2.8 2.290 +0.753 2.9 0.30 9.4 0.0 0.00 0.0 H 1702-429 256.520 -42.991 3.7 343.904 -1.265 15.0 0.00 6.8 0.0 0.00 0.0 SLX 1735-269 264.536 -27.024 4.2 0.754 +2.411 1.9 0.31 5.9 1.4 0.27 5.2 3A 1728-169 262.954 -16.993 4.2 8.496 +9.005 4.1 0.68 6.0 0.0 0.00 0.0 1E 1742.9-2849 266.504 -28.828 4.8 0.138 -0.018 1.4 0.27 5.1 0.0 0.00 0.0 SAX J1712.6-3739 258.222 -37.694 4.4 348.931 +0.846 3.3 0.58 5.7 0.0 0.00 0.0 SLX 1744-299_300 266.817 -29.915 5.1 359.350 -0.815 1.4 0.29 4.8 0.0 0.00 0.0 GRS 1734-292 264.340 -29.134 4.7 358.878 +1.428 1.6 0.30 5.3 0.0 0.00 0.0 1A 1742-294 266.414 -29.522 6.2 359.505 -0.312 1.1 0.28 3.9 0.0 0.00 0.0 XB 1832-330 278.971 -32.881 6.1 1.646 -11.354 2.5 0.63 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 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) +/- ==================== ======== ======== ======== ======== ====== ===== ====== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 3.4 0.33 0.9 0.20 GX 3+1 266.983 -26.564 2.294 +0.794 27.3 0.59 3.8 0.30 GX 5-1 270.284 -25.079 5.077 -1.019 95.4 2.27 12.4 1.04
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