INTEGRAL Galactic Bulge Monitoring Revolution 0729: Observation start 2008-10-02T04:48 = MJD 54741.2
Total Observation GTI = 12057 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 266.563 -32.233 0.5 357.254 -1.831 29.6 0.35 85.1 17.2 0.30 58.1 GX 354-0 262.992 -33.835 0.6 354.303 -0.152 24.6 0.36 68.9 7.5 0.30 24.7 GRS 1758-258 270.294 -25.745 1.1 4.503 -1.356 11.0 0.38 29.0 6.5 0.31 20.7 1E 1740.7-2942 265.968 -29.747 1.2 359.110 -0.099 9.1 0.35 26.1 6.0 0.30 20.0 GX 1+4 263.002 -24.754 1.2 1.926 +4.795 9.0 0.35 25.5 0.0 0.00 0.0 Ginga 1826-24 277.363 -23.792 1.3 9.275 -6.081 15.6 0.72 21.9 6.1 0.55 11.1 GX 349+2 256.438 -36.424 1.7 349.104 +2.746 9.6 0.57 16.8 0.0 0.00 0.0 SAX J1808.4-3658 272.105 -36.971 1.8 355.389 -8.138 8.1 0.52 15.5 3.7 0.42 8.8 GX 5-1 270.252 -25.081 2.1 5.061 -0.994 4.9 0.38 12.8 0.0 0.00 0.0 H 1820-303 275.912 -30.339 2.2 2.806 -7.899 6.5 0.53 12.4 0.0 0.00 0.0 3A 1822-371 276.456 -37.081 2.5 356.876 -11.288 7.6 0.72 10.5 0.0 0.00 0.0 4U 1722-30 261.915 -30.795 2.7 356.339 +2.283 3.5 0.37 9.6 1.5 0.00 5.1 GX 3+1 266.976 -26.551 2.7 2.301 +0.805 3.3 0.33 9.9 0.0 0.00 0.0 OAO 1657-415 255.131 -41.668 3.2 344.326 +0.355 10.6 1.33 8.0 3.6 1.02 3.6 SAX J1750.8-2900 267.615 -29.022 2.8 0.473 -0.951 2.8 0.30 9.2 0.0 0.00 0.0 SLX 1735-269 264.556 -26.932 4.1 0.841 +2.445 2.1 0.34 6.2 0.0 0.00 0.0 GX 9+1 270.386 -20.485 4.2 9.116 +1.174 3.0 0.50 6.0 0.0 0.00 0.0 4U 1700-377 256.054 -37.843 4.8 347.787 +2.132 3.4 0.65 5.2 0.0 0.00 0.0 H 1702-429 256.526 -42.960 5.2 343.930 -1.251 8.6 1.82 4.7 0.0 0.00 0.0 XB 1832-330 278.834 -32.971 6.2 1.513 -11.288 2.8 0.71 3.9 0.0 0.00 0.0 Swift J174535.5-2901 266.362 -29.028 5.5 359.902 -0.015 1.4 0.31 4.4 0.0 0.00 0.0 NEW_1 259.624 -13.731 3.9 9.547 +13.465 13.1 2.19 6.4 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 11.8 1.16 4.6 0.87 1A 1742-294 266.523 -29.515 359.559 -0.389 4.2 0.44 0.9 0.25 IGR J17464-3213 266.567 -32.229 357.260 -1.832 5.5 0.64 3.8 0.42 GX 3+1 266.983 -26.564 2.294 +0.794 47.9 0.69 7.1 0.38 GX 5-1 270.284 -25.079 5.077 -1.019 104.5 4.36 15.0 1.96
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