INTEGRAL Galactic bulge Monitoring
Revolution 1262: Observation start 2013-02-12T07:54 = MJD 56335.33
Total Observation GTI = 10943 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== Swift J174510.8-2624 266.301 -26.390 1.1 2.125 +1.406 12.0 0.44 27.2 8.4 0.30 27.6 4U 1700-377 255.998 -37.853 1.3 347.753 +2.161 20.5 0.92 22.3 5.0 0.59 8.4 Ginga 1826-24 277.352 -23.797 1.5 9.266 -6.076 15.0 0.79 19.0 6.1 0.54 11.3 Swift J1753.7-2544 268.419 -25.736 1.6 3.665 +0.111 7.8 0.43 18.0 5.7 0.30 18.7 GX 5-1 270.280 -25.086 1.6 5.070 -1.018 8.6 0.50 17.3 0.0 0.00 0.0 GRS 1758-258 270.306 -25.742 1.7 4.511 -1.364 7.4 0.45 16.4 6.3 0.31 20.3 OAO 1657-415 255.209 -41.668 1.7 344.362 +0.308 31.3 1.88 16.7 6.6 1.14 5.8 XTE J1810-189 272.600 -19.080 2.2 11.359 +0.043 10.3 0.82 12.6 2.9 0.55 5.3 GX 3+1 267.026 -26.538 2.7 2.336 +0.775 4.5 0.47 9.6 0.0 0.00 0.0 H 1820-303 275.888 -30.364 2.4 2.774 -7.891 7.2 0.66 10.9 0.0 0.00 0.0 GX 349+2 256.493 -36.431 4.0 349.126 +2.707 4.9 0.77 6.4 0.0 0.00 0.0 IGR J17091-3624 257.273 -36.336 4.3 349.578 +2.260 4.4 0.00 5.8 0.0 0.00 0.0 3A 1822-371 276.411 -37.045 0.0 356.893 -11.240 4.9 0.00 5.5 0.0 0.00 0.0 GRS 1747-312 267.678 -31.314 4.8 358.531 -2.171 2.3 0.00 5.1 0.0 0.00 0.0 4U 1722-30 261.897 -30.923 4.4 356.223 +2.225 2.8 0.50 5.6 1.7 0.34 5.0 KS 1741-293 266.226 -29.354 0.0 359.562 -0.084 2.1 0.00 4.7 0.0 0.00 0.0 IGR J17586-2129 269.514 -21.381 0.0 7.933 +1.436 2.9 0.00 4.5 0.0 0.00 0.0 SLX 1744-299_300 266.903 -30.046 4.0 359.276 -0.947 2.7 0.43 6.3 0.0 0.00 0.0 1RXS J175113.3-20121 267.866 -20.138 5.2 8.231 +3.393 3.2 0.67 4.7 0.0 0.00 0.0 GX 17+2 273.978 -14.099 0.0 16.364 +1.272 14.2 0.00 4.3 0.0 0.00 0.0 XTE J1743-363 265.687 -36.305 4.6 353.399 -3.338 2.8 0.53 5.4 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 1742-294 266.523 -29.515 359.559 -0.389 6.8 0.32 21.0 1.2 0.16 7.1 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.2 0.34 3.7 0.3 0.17 2.0 GX 3+1 266.976 -26.561 2.293 +0.800 56.0 0.59 95.6 6.7 0.25 26.7 GX 354-0 262.989 -33.835 354.302 -0.150 7.2 0.84 8.5 1.1 0.56 2.0 GX 5-1 270.282 -25.081 5.074 -1.018 131.7 2.18 60.3 13.6 0.93 14.6 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.0 0.54 3.8 0.4 0.24 1.8 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.2 0.30 7.4 0.5 0.16 3.1 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.0 0.32 3.1 0.2 0.16 1.3 XTE J1739-285 264.983 -28.499 359.716 +1.290 10.0 0.37 26.9 1.2 0.18 6.7 Swift J174510.8-2624 266.279 -26.407 2.101 +1.413 4.1 0.56 7.2 1.7 0.25 6.7 NEW SOURCE 272.197 -26.117 5.015 -3.030 16.0 3.23 4.9 0.0 0.00 0.0 NEW SOURCE 272.515 -26.699 4.641 -3.560 15.4 3.13 4.9 0.0 0.00 0.0 NEW SOURCE 270.089 -26.531 3.729 -1.586 3.7 0.89 4.2 1.3 0.43 3.0 NEW SOURCE 269.517 -26.962 3.100 -1.357 2.5 0.68 3.7 0.8 0.32 2.6 NEW SOURCE 267.863 -27.544 1.855 -0.382 1.5 0.42 3.6 0.5 0.20 2.6