INTEGRAL Galactic bulge Monitoring
Revolution 0488: Observation start 2006-10-11T23:35 = MJD 54019.983
Total Observation GTI = 12195 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 1700-377 255.988 -37.848 0.5 347.752 +2.170 68.2 0.74 92.2 18.2 0.55 33.1 GX 5-1 270.291 -25.082 0.6 5.078 -1.025 19.5 0.35 56.2 0.0 0.00 0.0 GX 1+4 263.012 -24.742 0.7 1.942 +4.795 17.3 0.35 49.6 0.0 0.00 0.0 Ginga 1826-24 277.376 -23.791 1.0 9.282 -6.092 18.5 0.62 29.9 5.2 0.47 10.9 H 1820-303 275.922 -30.353 1.0 2.797 -7.912 15.3 0.49 31.5 0.0 0.00 0.0 IGR J17497-2821 267.412 -28.352 1.3 0.957 -0.454 8.4 0.37 22.7 6.0 0.31 19.4 GRS 1758-258 270.298 -25.736 1.5 4.513 -1.355 7.7 0.40 19.5 5.3 0.32 16.5 1E 1740.7-2942 265.985 -29.740 1.3 359.123 -0.108 7.4 0.34 21.7 4.6 0.29 16.0 GX 349+2 256.451 -36.415 1.9 349.118 +2.743 8.7 0.60 14.5 0.0 0.00 0.0 4U 1722-30 261.893 -30.822 2.0 356.305 +2.283 5.1 0.38 13.3 1.4 0.30 4.6 GX 354-0 262.981 -33.823 1.8 354.308 -0.138 5.5 0.36 15.1 0.0 0.00 0.0 3A 1822-371 276.448 -37.109 2.1 356.848 -11.295 8.5 0.67 12.6 0.0 0.00 0.0 1A 1742-294 266.539 -29.531 2.8 359.553 -0.409 3.3 0.35 9.4 1.7 0.31 5.5 GX 3+1 267.030 -26.557 2.4 2.321 +0.762 3.6 0.32 11.2 0.0 0.00 0.0 GX 9+1 270.389 -20.534 3.2 9.074 +1.147 4.1 0.51 8.0 0.0 0.00 0.0 GRS 1734-292 264.364 -29.119 3.9 358.902 +1.419 2.1 0.33 6.4 0.0 0.00 0.0 IGR J17252-3616 261.339 -36.269 3.7 351.527 -0.374 3.1 0.46 6.8 0.0 0.00 0.0 IGR J18027-2016 270.732 -20.293 0.0 9.443 +0.987 2.7 0.00 5.7 0.0 0.00 0.0 SLX 1735-269 264.584 -26.998 4.2 0.799 +2.389 2.2 0.37 5.9 1.6 0.30 5.5 GX 17+2 274.001 -14.032 4.0 16.433 +1.283 24.1 3.87 6.2 0.0 0.00 0.0 1E 1742.8-2853 266.480 -28.910 4.5 0.057 -0.042 1.6 0.29 5.6 0.0 0.00 0.0 SLX 1744-299_300 266.818 -29.975 4.9 359.299 -0.847 1.6 0.33 5.0 0.0 0.00 0.0 3A 1728-169 262.941 -16.964 5.3 8.514 +9.031 3.2 0.69 4.6 0.0 0.00 0.0 IGR J17544-2619 268.546 -26.304 5.2 3.233 -0.276 1.5 0.32 4.7 0.0 0.00 0.0 GRS 1739-278 265.749 -27.743 5.8 0.714 +1.116 1.4 0.32 4.2 0.0 0.00 0.0 V1223 Sgr 283.700 -31.105 5.5 4.993 -14.285 8.3 1.89 4.4 0.0 0.00 0.0 H 1702-429 256.520 -43.037 6.0 343.867 -1.294 11.2 2.77 4.1 0.0 0.00 0.0 V2400 Oph 258.083 -24.178 6.1 359.886 +8.830 1.8 0.00 4.0 0.0 0.00 0.0
JEM-X
JEM-X1 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-X1 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 2.3 0.30 7.7 0.9 0.19 4.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.1 0.30 3.6 0.8 0.19 4.2 GX 1+4 263.009 -24.746 1.937 +4.795 1.1 1.05 1.1 2.4 0.72 3.3 GX 3+1 266.982 -26.569 2.289 +0.792 36.8 0.49 74.9 4.5 0.25 17.7 GX 354-0 262.989 -33.835 354.302 -0.150 22.9 1.33 17.2 4.9 1.01 4.9 GX 5-1 270.297 -25.079 5.083 -1.029 89.1 1.69 52.7 15.7 0.82 19.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.5 0.39 3.8 0.3 0.24 1.2 IGR J17497-2821 267.406 -28.359 0.948 -0.453 1.8 0.33 5.5 0.8 0.19 4.3 NEW SOURCE 271.759 -25.627 5.254 -2.449 9.0 2.23 4.0 1.4 1.19 1.1 NEW SOURCE 269.960 -26.632 3.584 -1.536 2.7 0.69 3.9 0.5 0.37 1.3 NEW SOURCE 267.155 -25.139 3.594 +1.397 2.6 0.67 3.9 0.0 0.00 0.0 NEW SOURCE 271.628 -25.897 4.960 -2.477 5.6 1.82 3.1 2.2 1.01 2.2