INTEGRAL Galactic bulge Monitoring
Revolution 0961: Observation start 2010-08-26T23:09 = MJD 55434.965
Total Observation GTI = 12388 seconds
IBIS/ISGRI
IBIS/ISGRI significance mosaic images. Left: IBIS/ISGRI 18-40 keV. Right: 40-100 keV
Sources 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
OSA10.1, of all the sources detected in the 18 - 40 keV range (band A: 1 Crab ~ 208 cps ) and 40 - 100 keV range (band B: 1 Crab ~ 100 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 and NEW SOURCEs < 6σ towards the border of the image may be spurious. IBIS/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 1700-377 255.981 -37.849 0.6 347.748 +2.174 47.9 0.73 66.0 15.1 0.54 27.8 GX 1+4 263.010 -24.742 1.0 1.940 +4.796 14.0 0.44 32.0 0.0 0.00 0.0 1E 1740.7-2942 265.988 -29.752 1.1 359.115 -0.116 10.8 0.37 29.3 7.5 0.30 25.4 GX 5-1 270.281 -25.086 1.3 5.070 -1.019 9.1 0.38 23.7 1.3 0.00 4.2 IGR J17464-3213 266.567 -32.237 1.2 357.253 -1.837 8.7 0.35 25.0 3.4 0.29 12.0 Ginga 1826-24 277.370 -23.784 1.6 9.285 -6.083 11.1 0.64 17.4 4.3 0.47 9.2 GRS 1758-258 270.302 -25.735 1.7 4.515 -1.358 5.9 0.36 16.6 3.1 0.29 10.9 GX 349+2 256.462 -36.431 2.0 349.110 +2.726 10.5 0.75 13.9 0.0 0.00 0.0 H 1820-303 275.913 -30.397 2.4 2.753 -7.926 5.7 0.50 11.4 0.0 0.00 0.0 OAO 1657-415 255.209 -41.664 2.2 344.365 +0.312 18.3 1.47 12.5 0.0 0.00 0.0 3A 1822-371 276.458 -37.101 2.5 356.858 -11.298 6.6 0.63 10.5 0.0 0.00 0.0 4U 1722-30 261.901 -30.788 2.5 356.338 +2.297 4.2 0.40 10.5 2.6 0.31 8.3 GX 354-0 263.025 -33.777 3.6 354.367 -0.144 3.0 0.43 7.1 0.0 0.00 0.0 SLX 1735-269 264.604 -26.991 3.5 0.814 +2.377 2.7 0.37 7.4 1.2 0.00 4.1 H 1705-440 257.381 -44.103 5.3 343.386 -2.432 8.4 1.82 4.6 0.0 0.00 0.0 IGR J17252-3616 261.219 -36.302 4.4 351.446 -0.312 2.8 0.49 5.7 1.6 0.38 4.3 1A 1742-294 266.547 -29.538 0.0 359.551 -0.419 1.9 0.00 5.4 0.0 0.00 0.0 GX 9+1 270.375 -20.542 4.2 9.061 +1.155 3.5 0.59 6.0 0.0 0.00 0.0 4U 1735-444 264.670 -44.473 5.3 346.007 -6.962 7.9 1.70 4.7 0.0 0.00 0.0 IGR J17285-2922 262.115 -29.361 5.1 357.630 +2.933 2.0 0.42 4.9 1.3 0.00 4.0 GX 3+1 266.974 -26.622 5.3 2.239 +0.770 1.7 0.36 4.7 0.0 0.00 0.0 Swift J174535.5-2901 266.360 -29.126 0.0 359.818 -0.065 1.6 0.00 4.2 0.0 0.00 0.0 IGR J18249-3243 276.253 -32.740 5.9 0.767 -9.235 1.9 0.00 4.1 0.0 0.00 0.0 IGR J16500-3307 252.618 -33.186 5.7 349.715 +7.212 4.1 0.95 4.3 0.0 0.00 0.0 IGR J18173-2509 274.457 -25.200 6.2 6.795 -4.386 1.8 0.46 3.9 0.0 0.00 0.0 XB 1832-330 278.994 -33.002 5.9 1.543 -11.423 2.6 0.61 4.2 1.9 0.00 4.1 XTE J1752-223 267.995 -22.260 6.4 6.462 +2.210 1.7 0.00 3.8 0.0 0.00 0.0
JEM-X
JEM-X2 significance mosaic images. Left: 3-10 keV. Right: 10-25 keV.
Sources labelled were detected in the 3-10 keV image > 6σ. The sources detected above 3σ in the 3-10 keV and/or 10-25 keV band 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 ~ 97 cps [J1], 103 cps [J2]); B = 10-25 keV (1 Crab ~ 29 cps [J1], 27 cps [J2]). NOTES: 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. The systematic noise increases towards the edge of the field of view and in the vicinity of very bright sources, such as GX 5-1;
NEW SOURCEs < 6σ towards the border of the image and/or near GX 5-1 may, therefore, be spurious.
JEM-X2 Detected Sources in 3-10 keV (A) and 10-25 keV (B).
Source Name RA dec l b A(cps) +/- sig B(cps) +/- sig ==================== ======== ======= ======== ======== ====== ===== ===== ====== ===== ===== 1A 1742-294 266.523 -29.515 359.559 -0.389 2.4 0.26 9.1 0.7 0.16 4.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.5 0.28 5.3 1.2 0.17 6.9 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.7 0.29 5.9 0.3 0.17 1.9 4U 1722-30 261.888 -30.802 356.320 +2.298 2.2 0.56 3.9 0.0 0.00 0.0 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.0 0.29 3.4 0.3 0.17 1.7 GX 3+1 266.983 -26.564 2.294 +0.794 16.6 0.53 31.6 1.5 0.28 5.2 GX 354-0 262.989 -33.830 354.306 -0.147 15.7 0.88 17.9 2.5 0.54 4.6 GX 5-1 270.287 -25.072 5.085 -1.017 117.6 2.14 55.1 14.4 1.12 12.9 IGR J17464-3213 266.567 -32.229 357.260 -1.832 8.8 0.30 29.2 1.3 0.18 7.1 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.4 0.27 8.9 0.5 0.16 3.3 NEW SOURCE 266.524 -24.003 4.270 +2.475 9.7 2.16 4.5 0.0 0.00 0.0 NEW SOURCE 266.628 -25.552 2.994 +1.591 2.8 0.73 3.8 0.8 0.40 2.1 NEW SOURCE 270.696 -25.515 4.882 -1.557 6.7 1.56 4.3 1.3 0.87 1.5 NEW SOURCE 273.098 -27.521 4.167 -4.409 7.4 1.54 4.8 0.0 0.00 0.0 NEW SOURCE 267.058 -24.906 3.749 +1.592 3.1 1.01 3.1 1.5 0.57 2.6