INTEGRAL Galactic bulge Monitoring
Revolution 1329: Observation start 2013-08-31T20:37 = MJD 56535.86
Total Observation GTI = 10099 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GX 354-0 262.989 -33.827 0.8 354.308 -0.146 17.5 0.43 40.9 6.4 0.30 21.5 Ginga 1826-24 277.366 -23.805 1.2 9.265 -6.090 17.3 0.68 25.4 7.5 0.45 16.7 GX 5-1 270.281 -25.078 1.2 5.077 -1.015 11.1 0.42 26.2 0.0 0.00 0.0 GRS 1758-258 270.326 -25.745 1.2 4.517 -1.381 10.9 0.43 25.5 8.4 0.30 28.3 IGR J17464-3213 266.575 -32.242 1.4 357.252 -1.844 8.1 0.40 20.2 4.2 0.29 14.4 H 1820-303 275.913 -30.374 2.0 2.774 -7.915 7.4 0.54 13.7 0.0 0.00 0.0 GX 1+4 262.991 -24.738 2.2 1.935 +4.813 5.5 0.45 12.2 0.0 0.00 0.0 3A 1822-371 276.436 -37.108 2.8 356.845 -11.285 6.6 0.70 9.5 0.0 0.00 0.0 GX 349+2 256.464 -36.453 2.8 349.093 +2.712 6.4 0.68 9.4 0.0 0.00 0.0 GX 9+1 270.415 -20.478 3.7 9.135 +1.154 4.0 0.58 6.9 0.0 0.00 0.0 Swift J1734.5-3027 263.557 -30.343 3.4 357.493 +1.349 2.8 0.37 7.6 1.2 0.26 4.7 OAO 1657-415 255.237 -41.667 3.1 344.376 +0.293 12.4 1.49 8.3 5.1 0.98 5.2 SLX 1735-269 264.562 -26.892 4.1 0.878 +2.461 2.4 0.39 6.2 1.4 0.27 5.1 KS 1741-293 266.232 -29.333 4.5 359.582 -0.078 1.9 0.33 5.6 0.0 0.00 0.0 GX 13+1 273.635 -17.261 4.3 13.427 +0.054 6.3 1.08 5.8 0.0 0.00 0.0 GX 3+1 266.954 -26.549 4.8 2.293 +0.824 2.0 0.00 5.2 0.0 0.00 0.0 1E 1740.7-2942 266.000 -29.809 5.8 359.071 -0.155 1.4 0.34 4.2 0.0 0.00 0.0 SLX 1744-299_300 266.912 -30.100 5.9 359.235 -0.981 1.4 0.33 4.1 0.0 0.00 0.0 IGR J17252-3616 261.245 -36.198 5.7 351.544 -0.271 2.1 0.00 4.3 0.0 0.00 0.0 IGR J17586-2129 269.639 -21.469 0.0 7.915 +1.291 2.1 0.00 4.1 1.5 0.00 4.2 GX 17+2 274.058 -14.061 6.0 16.435 +1.221 24.7 6.11 4.0 0.0 0.00 0.0 XTE J1720-318 259.944 -31.822 5.9 354.540 +3.097 1.9 0.46 4.1 0.0 0.00 0.0 GRS 1734-292 264.353 -29.180 5.2 358.845 +1.394 1.7 0.35 4.8 0.0 0.00 0.0 NEW SOURCE 270.553 -34.999 3.8 356.532 -6.093 3.0 0.45 6.6 0.0 0.00 0.0 NEW SOURCE 258.808 -31.718 4.0 354.068 +3.946 3.1 0.48 6.3 0.0 0.00 0.0 NEW SOURCE 271.170 -31.697 3.9 359.683 -4.943 2.9 0.44 6.5 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined 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+2 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 1742-294 266.526 -29.523 359.554 -0.396 8.2 0.23 35.5 1.4 0.13 11.5 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 0.7 0.22 3.2 0.0 0.00 0.0 4U 1722-30 261.901 -30.802 356.326 +2.290 7.7 0.38 20.2 1.2 0.23 5.0 GX 3+1 266.992 -26.566 2.296 +0.786 43.9 0.51 86.4 4.5 0.25 18.0 GX 354-0 262.989 -33.835 354.302 -0.150 12.6 0.76 16.5 3.6 0.53 6.9 GX 5-1 270.285 -25.082 5.075 -1.021 125.6 1.86 67.6 18.1 0.81 22.2 IGR J17464-3213 266.567 -32.229 357.260 -1.832 4.9 0.30 16.5 1.2 0.17 6.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.6 0.23 7.3 0.5 0.13 3.9 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.5 0.24 6.4 0.2 0.13 1.8 NEW SOURCE 270.363 -24.293 5.796 -0.691 12.4 2.36 5.3 1.6 1.15 1.4 NEW SOURCE 272.565 -26.124 5.168 -3.324 12.8 2.47 5.2 2.4 1.37 1.7 NEW SOURCE 270.761 -25.516 4.910 -1.609 7.6 1.53 5.0 0.9 0.67 1.4 NEW SOURCE 270.037 -24.018 5.887 -0.296 12.4 2.74 4.5 0.0 0.00 0.0 NEW SOURCE 268.120 -23.666 5.309 +1.396 12.1 2.40 5.0 2.2 1.34 1.6 NEW SOURCE 270.816 -23.866 6.371 -0.841 17.1 3.71 4.6 0.0 0.00 0.0 NEW SOURCE 271.101 -25.403 5.159 -1.821 6.1 1.75 3.5 2.1 0.85 2.4