INTEGRAL Galactic bulge Monitoring
Revolution 1392: Observation start 2014-03-10T03:40 = MJD 56726.154
Total Observation GTI = 13462 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== GRO J1744-28 266.138 -28.742 0.2 0.044 +0.300 131.7 0.34 387.6 13.1 0.21 62.1 4U 1700-377 255.976 -37.843 0.8 347.751 +2.181 30.3 0.77 39.2 10.7 0.44 24.2 GRS 1758-258 270.301 -25.738 1.1 4.513 -1.358 12.1 0.43 28.4 9.7 0.25 38.9 Ginga 1826-24 277.370 -23.788 1.1 9.282 -6.086 18.8 0.66 28.4 7.4 0.37 19.8 GX 5-1 270.278 -25.079 1.3 5.075 -1.013 10.2 0.43 23.7 0.0 0.00 0.0 GX 1+4 263.026 -24.780 2.1 1.917 +4.763 5.6 0.42 13.3 0.0 0.00 0.0 H 1820-303 275.899 -30.365 2.0 2.777 -7.900 8.2 0.59 14.0 0.0 0.00 0.0 GX 17+2 274.009 -14.021 2.2 16.447 +1.283 27.3 2.19 12.4 0.0 0.00 0.0 3A 1822-371 276.492 -37.092 2.8 356.879 -11.319 7.2 0.77 9.3 0.0 0.00 0.0 GX 354-0 262.978 -33.835 2.5 354.297 -0.142 4.1 0.38 10.6 0.0 0.00 0.0 SLX 1735-269 264.542 -26.953 3.1 0.817 +2.445 3.1 0.36 8.4 1.2 0.22 5.2 GX 3+1 266.958 -26.563 3.0 2.282 +0.813 3.2 0.38 8.5 0.0 0.00 0.0 GX 349+2 256.479 -36.408 3.6 349.136 +2.730 5.1 0.73 7.0 0.0 0.00 0.0 KS 1741-293 266.223 -29.248 0.0 359.651 -0.027 2.2 0.00 6.3 0.0 0.00 0.0 GX 9+1 270.412 -20.527 4.0 9.091 +1.132 3.4 0.00 6.2 0.0 0.00 0.0 1E 1742.8-2853 266.506 -28.919 0.0 0.060 -0.067 2.1 0.00 6.0 0.0 0.00 0.0 4U 1722-30 261.883 -30.770 3.6 356.344 +2.320 3.1 0.43 7.2 1.0 0.25 4.0 1E 1740.7-2942 266.033 -29.741 0.0 359.144 -0.144 2.0 0.00 5.5 1.0 0.23 4.5 SLX 1744-299_300 266.887 -30.070 0.0 359.249 -0.947 2.0 0.00 5.1 0.0 0.00 0.0 GRS 1739-278 265.669 -27.683 0.0 0.728 +1.208 1.7 0.00 4.9 0.0 0.00 0.0 IGR J17597-2201 269.915 -22.019 5.4 7.566 +0.794 2.2 0.49 4.6 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 6.4 0.31 20.6 1.0 0.18 5.4 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.1 0.30 3.6 0.4 0.18 2.5 GRO J1744-28 266.136 -28.735 0.048 +0.306 76.3 0.35 221.1 34.4 0.20 168.5 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.4 0.30 4.8 0.4 0.17 2.3 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.3 0.85 2.7 1.4 0.42 3.4 GX 1+4 263.009 -24.746 1.937 +4.795 2.6 0.73 3.5 1.3 0.43 3.1 GX 3+1 266.983 -26.570 2.288 +0.791 46.5 0.39 119.1 4.1 0.20 20.7 GX 354-0 262.989 -33.835 354.302 -0.150 24.5 1.72 14.2 2.4 1.38 1.8 GX 5-1 270.284 -25.079 5.077 -1.019 155.0 1.20 128.8 15.2 0.53 28.6 SLX 1735-269 264.571 -26.994 0.796 +2.400 3.2 0.35 9.2 1.2 0.20 5.8 NEW SOURCE 265.842 -29.769 359.034 -0.017 2.1 0.30 7.1 0.5 0.18 2.8 NEW SOURCE 267.627 -31.366 358.464 -2.160 2.4 0.43 5.5 0.7 0.26 2.8 NEW SOURCE 271.392 -28.347 2.714 -3.484 3.8 0.76 5.0 0.0 0.00 0.0 NEW SOURCE 271.026 -26.679 4.013 -2.388 4.6 0.81 5.7 0.4 0.40 1.1 NEW SOURCE 267.139 -33.900 356.075 -3.106 2.8 0.96 2.9 2.8 0.69 4.1 NEW SOURCE 266.630 -32.302 357.225 -1.916 2.2 0.49 4.5 1.2 0.32 3.9 AX J1754.2-2754 268.579 -27.912 1.860 -1.115 0.7 0.37 1.9 0.8 0.20 3.9 NEW SOURCE 267.746 -33.698 356.507 -3.436 2.1 0.92 2.3 2.5 0.68 3.7