INTEGRAL Galactic Bulge Monitoring Revolution 0730: Observation start 2008-10-04T21:56 = MJD 54743.915
Total Observation GTI = 11273 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== IGR J17464-3213 266.567 -32.232 0.4 357.257 -1.834 33.9 0.35 97.9 18.7 0.29 63.5 GX 354-0 262.991 -33.833 0.6 354.304 -0.151 26.6 0.39 69.0 8.2 0.32 25.6 4U 1700-377 255.980 -37.841 0.6 347.754 +2.179 40.1 0.68 58.6 10.4 0.53 19.5 1E 1740.7-2942 265.988 -29.744 1.1 359.121 -0.112 9.6 0.35 27.6 6.1 0.30 20.5 GRS 1758-258 270.302 -25.742 1.3 4.509 -1.361 8.8 0.39 22.9 7.0 0.31 22.3 GX 1+4 263.019 -24.746 1.3 1.942 +4.787 9.6 0.41 23.6 0.0 0.00 0.0 Ginga 1826-24 277.355 -23.808 1.3 9.257 -6.082 16.7 0.74 22.8 5.9 0.57 10.3 GX 349+2 256.431 -36.422 1.5 349.102 +2.752 10.7 0.55 19.5 0.0 0.00 0.0 GX 5-1 270.276 -25.091 1.7 5.064 -1.018 6.9 0.41 16.8 0.0 0.00 0.0 H 1820-303 275.939 -30.384 1.5 2.775 -7.940 9.5 0.51 18.6 0.0 0.00 0.0 3A 1822-371 276.458 -37.119 2.0 356.842 -11.306 8.7 0.65 13.5 0.0 0.00 0.0 GX 3+1 267.008 -26.569 2.2 2.301 +0.772 4.9 0.39 12.5 0.0 0.00 0.0 SAX J1808.4-3658 272.085 -36.994 2.1 355.361 -8.134 6.2 0.48 12.9 1.9 0.00 4.9 SAX J1750.8-2900 267.628 -29.039 3.0 0.465 -0.969 2.7 0.32 8.5 0.0 0.00 0.0 4U 1722-30 261.886 -30.775 2.7 356.342 +2.315 3.7 0.38 9.9 1.6 0.29 5.4 OAO 1657-415 255.232 -41.633 3.1 344.401 +0.317 9.6 1.16 8.2 4.7 0.90 5.2 GX 9+1 270.448 -20.509 3.9 9.123 +1.112 3.8 0.60 6.5 0.0 0.00 0.0 SLX 1735-269 264.608 -26.973 3.8 0.832 +2.384 2.5 0.37 6.7 1.6 0.31 5.4 SLX 1744-299_300 266.853 -30.054 4.2 359.248 -0.914 1.9 0.32 6.0 0.0 0.00 0.0 4U 1705-32 257.300 -32.356 5.4 352.798 +4.608 2.0 0.44 4.6 0.0 0.00 0.0 1A 1742-294 266.552 -29.599 4.6 359.500 -0.455 1.9 0.36 5.4 0.0 0.00 0.0 H 1702-429 256.462 -43.045 5.1 343.835 -1.264 7.2 0.00 4.8 0.0 0.00 0.0 MXB 1730-335 263.376 -33.435 0.0 354.813 -0.202 1.6 0.00 4.6 0.0 0.00 0.0 GX 17+2 274.065 -14.004 4.9 16.488 +1.242 42.5 8.34 5.1 0.0 0.00 0.0 IGR J17473-2721 266.857 -27.336 4.5 1.574 +0.491 1.9 0.34 5.5 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 8.8 0.74 3.6 0.51 1A 1742-294 266.523 -29.515 359.559 -0.389 2.5 0.41 0.7 0.27 IGR J17464-3213 266.567 -32.229 357.260 -1.832 6.3 0.45 4.1 0.33 GX 3+1 266.983 -26.564 2.294 +0.794 42.5 0.93 6.4 0.50 GX 5-1 270.284 -25.079 5.077 -1.019 78.3 5.43 7.0 2.37
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