INTEGRAL Galactic bulge Monitoring
Revolution 0849: Observation start 2009-09-27T13:13 = MJD 55101.551
Total Observation GTI = 12294 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 1700-377 255.992 -37.846 0.6 347.755 +2.169 52.0 0.92 56.5 12.8 0.70 18.3 1E 1740.7-2942 265.981 -29.740 0.9 359.122 -0.105 12.2 0.34 35.7 8.3 0.29 28.6 GRS 1758-258 270.315 -25.718 1.2 4.536 -1.359 8.7 0.34 25.7 5.3 0.29 18.7 Ginga 1826-24 277.378 -23.781 1.2 9.291 -6.089 13.7 0.56 24.4 5.4 0.45 12.0 GX 1+4 262.979 -24.742 2.0 1.925 +4.820 5.0 0.37 13.4 0.0 0.00 0.0 OAO 1657-415 255.206 -41.640 2.2 344.383 +0.327 26.1 2.14 12.2 11.2 1.63 6.9 GX 5-1 270.289 -25.092 2.2 5.068 -1.029 4.4 0.36 12.4 0.0 0.00 0.0 IGR J17586-2129 269.685 -21.383 2.5 8.011 +1.296 4.8 0.45 10.6 0.0 0.00 0.0 IGR J17511-3057 267.801 -30.999 2.8 358.856 -2.100 3.5 0.37 9.5 0.0 0.00 0.0 4U 1722-30 261.875 -30.798 3.0 356.317 +2.310 3.9 0.45 8.7 1.8 0.36 4.9 3A 1822-371 276.446 -37.057 3.5 356.895 -11.271 4.1 0.57 7.3 0.0 0.00 0.0 H 1820-303 275.883 -30.362 3.2 2.773 -7.887 3.9 0.48 8.1 0.0 0.00 0.0 GX 349+2 256.439 -36.419 3.2 349.109 +2.748 5.8 0.73 8.0 0.0 0.00 0.0 GX 3+1 266.980 -26.551 4.2 2.303 +0.803 2.1 0.34 6.0 0.0 0.00 0.0 Swift J175759.9-2246 269.434 -22.842 5.7 6.630 +0.769 1.7 0.40 4.3 0.0 0.00 0.0 GX 9+1 270.343 -20.423 4.8 9.149 +1.240 2.8 0.53 5.2 0.0 0.00 0.0 1A 1743-288 266.680 -28.827 4.0 0.218 -0.149 2.0 0.31 6.3 0.0 0.00 0.0 XB 1832-330 278.906 -32.967 4.7 1.543 -11.341 3.0 0.57 5.3 0.0 0.00 0.0 GX 17+2 274.044 -14.011 5.6 16.472 +1.257 13.6 3.07 4.4 0.0 0.00 0.0 SLX 1735-269 264.628 -27.034 4.9 0.789 +2.337 2.0 0.40 5.0 0.0 0.00 0.0 SLX 1744-299_300 266.807 -29.987 6.2 359.284 -0.845 1.3 0.33 3.9 0.0 0.00 0.0 IGR J17544-2619 268.528 -26.370 6.3 3.167 -0.296 1.3 0.34 3.8 0.0 0.00 0.0 HETE J1900.1-2455 285.005 -24.949 5.5 11.267 -12.859 12.5 2.80 4.5 0.0 0.00 0.0 Oph Cluster 258.026 -23.317 6.0 0.569 +9.368 2.6 0.00 4.0 0.0 0.00 0.0 1A 1742-294 266.536 -29.606 6.7 359.488 -0.446 1.2 0.00 3.6 0.0 0.00 0.0 3A 1728-169 262.906 -17.048 5.3 8.424 +9.015 4.0 0.86 4.7 0.0 0.00 0.0 IGR J17375-3022 264.420 -30.491 7.6 357.769 +0.642 1.2 0.40 3.1 0.0 0.00 0.0 GRS 1747-312 267.766 -31.338 0.0 358.549 -2.247 1.2 0.00 3.4 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 5.5 0.29 19.2 1.1 0.18 5.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.2 0.29 7.3 1.8 0.21 8.5 GX 3+1 266.980 -26.565 2.291 +0.795 27.9 0.48 58.7 3.2 0.25 12.5 GX 5-1 270.289 -25.067 5.090 -1.016 91.2 1.14 80.3 5.8 0.51 11.3 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.4 0.51 4.6 0.4 0.32 1.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.27 4.0 0.3 0.19 1.6 XTE J1739-285 264.975 -28.496 359.714 +1.298 1.3 0.37 3.5 0.0 0.00 0.0 CONFUSED ID 270.287 -25.082 5.076 -1.022 98.5 1.15 85.7 6.3 0.51 12.2 IGR J17511-3057 267.785 -30.954 358.888 -2.065 1.7 0.27 6.3 0.6 0.20 2.9 NEW SOURCE 272.762 -26.187 5.198 -3.509 6.8 1.24 5.5 1.1 0.73 1.6 CONFUSED ID 270.373 -25.063 5.131 -1.081 21.2 1.00 21.2 1.4 0.49 2.8 NEW SOURCE 267.503 -24.225 4.541 +1.595 5.2 1.05 5.0 0.0 0.00 0.0 NEW SOURCE 270.118 -24.264 5.711 -0.483 6.6 1.41 4.7 0.0 0.00 0.0