INTEGRAL Galactic bulge Monitoring
Revolution 1469: Observation start 2014-10-26T00:31 = MJD 56956.022
Total Observation GTI = 12154 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 1700-377 255.989 -37.846 0.4 347.754 +2.171 78.1 0.72 107.8 26.4 0.46 57.1 IGR J17464-3213 266.573 -32.234 0.9 357.258 -1.839 11.9 0.34 35.4 9.9 0.24 41.9 GRS 1758-258 270.308 -25.749 1.1 4.506 -1.368 10.9 0.41 26.4 8.9 0.28 32.3 Ginga 1826-24 277.354 -23.805 1.1 9.260 -6.080 16.7 0.63 26.3 6.8 0.42 16.4 GX 5-1 270.311 -25.098 1.9 5.072 -1.049 5.4 0.38 14.2 0.0 0.00 0.0 IGR J17454-2919 266.334 -29.293 2.0 359.663 -0.133 5.0 0.35 14.0 3.1 0.26 11.9 H 1820-303 275.913 -30.370 2.4 2.779 -7.913 5.9 0.52 11.3 0.0 0.00 0.0 SLX 1735-269 264.527 -26.994 2.8 0.775 +2.434 3.1 0.34 9.2 2.1 0.24 8.7 GRS 1739-278 265.700 -27.815 3.2 0.631 +1.115 3.0 0.37 8.0 1.7 0.27 6.6 GX 349+2 256.373 -36.435 3.2 349.064 +2.781 5.2 0.65 8.0 0.0 0.00 0.0 GX 354-0 262.987 -33.828 3.5 354.307 -0.146 2.9 0.40 7.3 0.0 0.00 0.0 3A 1822-371 276.551 -37.069 4.1 356.921 -11.351 4.5 0.00 6.1 0.0 0.00 0.0 SLX 1744-299_300 266.812 -29.993 4.2 359.281 -0.852 2.0 0.33 5.9 0.0 0.00 0.0 GX 3+1 266.915 -26.642 4.9 2.195 +0.806 1.8 0.36 5.0 0.0 0.00 0.0 1E 1740.7-2942 266.022 -29.751 0.0 359.131 -0.142 1.9 0.00 5.8 1.2 0.00 5.0 IGR J17456-2901 266.402 -28.929 0.0 0.004 +0.006 1.9 0.00 5.6 0.9 0.00 3.6 GX 9+1 270.344 -20.498 5.0 9.085 +1.202 2.4 0.48 5.0 0.0 0.00 0.0 GX 1+4 262.927 -24.721 5.4 1.917 +4.871 1.7 0.39 4.5 0.0 0.00 0.0 IGR J18214-1318 275.367 -13.360 5.0 17.653 +0.433 25.3 5.09 5.0 0.0 0.00 0.0 IGR J18027-1455 270.687 -14.911 4.4 14.112 +3.669 9.3 1.61 5.7 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 ~ 109 cps [J1], 116 cps [J2]); B = 10-25 keV (1 Crab ~ 34 cps [J1], 32 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 1742-294 266.515 -29.504 359.565 -0.378 6.3 0.24 26.5 1.1 0.13 7.9 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 0.8 0.23 3.6 0.4 0.14 2.8 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.24 3.7 0.2 0.13 1.7 4U 1722-30 261.888 -30.802 356.320 +2.298 2.5 0.48 5.2 0.7 0.32 2.1 GRS 1739-278 265.673 -27.738 0.683 +1.176 9.9 0.28 35.9 0.5 0.15 3.4 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.3 0.88 2.6 1.9 0.45 4.3 GX 3+1 266.982 -26.574 2.284 +0.789 29.6 0.37 80.4 3.2 0.19 17.1 GX 354-0 262.994 -33.836 354.303 -0.155 18.4 0.97 18.9 4.4 0.70 6.2 GX 5-1 270.288 -25.077 5.081 -1.020 121.5 1.45 84.0 12.2 0.66 18.5 IGR J17464-3213 266.567 -32.229 357.260 -1.832 2.9 0.33 8.7 1.5 0.21 7.3 SLX 1735-269 264.571 -26.994 0.796 +2.400 2.0 0.31 6.5 0.6 0.18 3.4 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.5 0.23 6.2 0.3 0.14 2.1 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.4 0.24 1.6 0.5 0.14 3.5 1A 1743-288 266.770 -28.874 0.220 -0.241 2.0 0.24 8.1 0.0 0.00 0.0 IGR J17454-2919 266.365 -29.333 359.643 -0.176 1.7 0.23 7.4 0.7 0.13 5.0 NEW SOURCE 271.450 -25.684 5.068 -2.233 7.5 1.49 5.0 1.4 0.80 1.8 NEW SOURCE 270.387 -23.861 6.182 -0.497 12.3 2.35 5.2 1.6 1.35 1.2 NEW SOURCE 270.727 -24.643 5.655 -1.153 5.5 1.65 3.4 1.9 0.86 2.3