INTEGRAL Galactic bulge Monitoring
Revolution 1265: Observation start 2013-02-22T15:22 = MJD 56345.641
Total Observation GTI = 12215 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 354-0 263.001 -33.828 1.0 354.313 -0.154 12.5 0.39 32.2 5.1 0.28 18.1 Swift J174510.8-2624 266.291 -26.412 1.1 2.101 +1.402 9.8 0.34 28.9 6.7 0.26 26.1 GRS 1758-258 270.301 -25.749 1.2 4.503 -1.364 8.9 0.37 24.2 6.3 0.27 23.5 GX 5-1 270.303 -25.078 1.4 5.087 -1.032 7.6 0.37 20.3 0.0 0.00 0.0 XTE J1810-189 272.602 -19.070 1.6 11.369 +0.046 10.4 0.59 17.7 3.8 0.42 9.1 Ginga 1826-24 277.358 -23.795 1.6 9.270 -6.079 11.5 0.64 17.9 5.6 0.44 12.7 4U 1700-377 255.932 -37.836 2.1 347.734 +2.213 9.8 0.75 13.0 4.4 0.53 8.3 4U 1722-30 261.889 -30.807 2.9 356.315 +2.295 3.5 0.39 8.9 1.1 0.00 4.0 KS 1741-293 266.242 -29.349 2.8 359.573 -0.094 3.0 0.32 9.5 1.7 0.24 6.9 GX 3+1 266.983 -26.543 2.9 2.311 +0.805 2.9 0.33 8.9 0.0 0.00 0.0 H 1820-303 275.906 -30.403 2.9 2.745 -7.922 4.2 0.47 8.9 0.0 0.00 0.0 Swift J1753.7-2544 268.312 -25.798 3.8 3.562 +0.161 2.2 0.32 6.7 1.3 0.24 5.5 GX 1+4 262.998 -24.744 3.5 1.934 +4.804 3.0 0.40 7.4 0.0 0.00 0.0 GX 9+1 270.368 -20.538 3.9 9.061 +1.162 2.9 0.45 6.5 0.0 0.00 0.0 XTE J1739-285 264.900 -28.435 3.6 359.731 +1.386 2.2 0.31 7.0 0.0 0.00 0.0 SLX 1735-269 264.515 -26.985 4.7 0.777 +2.448 1.8 0.33 5.3 0.0 0.00 0.0 3A 1822-371 276.477 -37.071 3.3 356.893 -11.299 6.2 0.80 7.8 0.0 0.00 0.0 OAO 1657-415 255.234 -41.744 4.5 344.314 +0.247 9.5 1.71 5.6 0.0 0.00 0.0 H 1702-429 256.572 -43.058 4.4 343.872 -1.337 18.4 3.27 5.6 0.0 0.00 0.0 SAX J1712.6-3739 258.105 -37.625 4.2 348.932 +0.962 3.7 0.62 6.0 0.0 0.00 0.0 GX 349+2 256.426 -36.412 4.8 349.108 +2.761 3.2 0.00 5.1 0.0 0.00 0.0 IGR J17091-3624 257.261 -36.432 5.6 349.495 +2.211 2.5 0.57 4.4 2.3 0.40 5.6 SAX J1806.5-2215 271.683 -22.263 5.0 8.159 -0.751 2.1 0.00 4.9 0.0 0.00 0.0 IGR J18173-2509 274.424 -25.076 5.7 6.891 -4.302 2.0 0.00 4.3 0.0 0.00 0.0 XTE J1752-223 268.037 -22.265 5.8 6.478 +2.174 1.6 0.37 4.2 0.0 0.00 0.0 IGR J17252-3616 261.344 -36.239 0.0 351.554 -0.361 1.9 0.00 4.1 0.0 0.00 0.0 IGR J17456-2901 266.388 -28.994 0.0 359.943 -0.018 1.2 0.00 3.9 0.0 0.00 0.0 1RXS J180408.9-34205 271.141 -34.390 0.0 357.302 -6.222 1.7 0.00 3.8 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 1742-294 266.514 -29.502 359.567 -0.376 7.0 0.28 24.9 1.1 0.14 8.0 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.27 3.0 0.2 0.13 1.7 4U 1722-30 261.888 -30.802 356.320 +2.298 3.1 0.59 5.3 1.3 0.36 3.4 GX 3+1 266.978 -26.562 2.293 +0.799 61.9 0.38 164.2 6.9 0.16 42.6 GX 354-0 262.989 -33.835 354.302 -0.150 8.3 1.50 5.5 3.9 1.34 2.9 GX 5-1 270.284 -25.079 5.077 -1.019 136.9 1.13 121.0 13.0 0.44 29.3 KS 1741-293 266.213 -29.365 359.546 -0.081 1.3 0.27 4.9 0.5 0.14 3.6 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.2 0.31 6.9 0.4 0.16 2.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.0 0.29 3.4 0.3 0.15 2.0 XTE J1739-285 264.931 -28.495 359.694 +1.331 10.1 0.28 36.0 1.3 0.14 9.0 Swift J174510.8-2624 266.284 -26.398 2.110 +1.415 2.8 0.34 8.2 1.3 0.16 8.2 NEW SOURCE 270.015 -26.054 0.000 +0.000 4.1 0.67 6.1 0.6 0.30 2.0 NEW SOURCE 269.353 -27.539 2.528 -1.519 2.6 0.42 6.1 0.0 0.00 0.0 NEW SOURCE 272.331 -25.480 5.632 -2.829 11.6 2.25 5.1 0.0 0.00 0.0 NEW SOURCE 272.928 -26.981 4.571 -4.019 7.6 1.64 4.6 3.0 1.02 2.9 NEW SOURCE 267.696 -27.004 2.243 +0.021 1.6 0.33 4.8 0.0 0.00 0.0 NEW SOURCE 272.934 -26.962 4.589 -4.014 7.5 1.65 4.5 3.2 1.03 3.1 NEW SOURCE 269.060 -24.261 5.231 +0.354 3.6 0.96 3.8 1.0 0.40 2.4