INTEGRAL Galactic bulge Monitoring
Revolution 0489: Observation start 2006-10-17T02:50 = MJD 54025.118
Total Observation GTI = 12102 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 1+4 263.007 -24.744 0.6 1.937 +4.798 25.5 0.39 65.8 0.0 0.00 0.0 4U 1700-377 255.986 -37.850 0.7 347.749 +2.171 35.5 0.69 51.8 9.0 0.52 17.5 GX 354-0 262.994 -33.834 0.8 354.304 -0.153 16.2 0.40 40.7 3.9 0.32 12.4 GX 5-1 270.283 -25.070 0.9 5.085 -1.013 14.3 0.39 36.3 0.0 0.00 0.0 GX 349+2 256.443 -36.427 1.0 349.104 +2.741 19.0 0.61 31.3 0.0 0.00 0.0 Ginga 1826-24 277.366 -23.795 1.1 9.273 -6.085 17.1 0.59 29.0 7.0 0.45 15.5 GRS 1758-258 270.311 -25.741 1.3 4.514 -1.367 7.8 0.33 23.4 5.6 0.27 20.7 1E 1740.7-2942 265.973 -29.754 1.3 359.105 -0.106 7.7 0.32 23.7 4.8 0.26 18.2 H 1820-303 275.929 -30.356 1.2 2.797 -7.919 11.6 0.49 23.8 0.0 0.00 0.0 IGR J17497-2821 267.389 -28.354 1.5 0.945 -0.438 6.6 0.35 18.7 3.9 0.29 13.5 4U 1722-30 261.883 -30.785 2.3 356.331 +2.311 3.9 0.34 11.5 2.1 0.27 7.7 3A 1822-371 276.438 -37.110 2.2 356.844 -11.288 8.3 0.66 12.5 0.0 0.00 0.0 GX 3+1 266.987 -26.587 2.7 2.275 +0.779 3.0 0.31 9.7 0.0 0.00 0.0 1A 1742-294 266.494 -29.502 0.0 359.557 -0.361 3.3 0.00 9.3 0.0 0.00 0.0 GX 9+1 270.399 -20.558 3.0 9.058 +1.128 4.6 0.52 8.8 0.0 0.00 0.0 GX 13+1 273.647 -17.179 4.2 13.505 +0.083 5.0 0.83 6.0 0.0 0.00 0.0 SLX 1735-269 264.577 -26.956 3.7 0.831 +2.417 2.4 0.35 6.9 1.3 0.29 4.4 SLX 1744-299_300 266.970 -29.995 4.6 359.350 -0.970 1.7 0.00 5.4 0.0 0.00 0.0 OAO 1657-415 255.211 -41.647 4.4 344.380 +0.321 9.6 1.68 5.7 0.0 0.00 0.0 IGR J18027-2016 270.731 -20.298 0.0 9.438 +0.986 2.6 0.00 5.2 0.0 0.00 0.0 IGR J16500-3307 252.455 -33.144 5.5 349.661 +7.345 3.3 0.00 4.5 0.0 0.00 0.0 GRO J1750-27 267.320 -26.621 0.0 2.400 +0.507 1.3 0.00 4.2 0.0 0.00 0.0 V2400 Oph 258.153 -24.266 6.0 359.850 +8.727 2.0 0.48 4.1 0.0 0.00 0.0 Swift J175648.6-2544 269.165 -25.684 6.4 4.049 -0.444 1.2 0.32 3.8 0.0 0.00 0.0 IGR J17195-4100 259.965 -40.918 6.7 347.087 -2.122 3.3 0.90 3.6 0.0 0.00 0.0 GX 17+2 273.970 -14.007 5.4 16.441 +1.322 17.1 3.77 4.5 0.0 0.00 0.0 Oph Cluster 258.062 -23.290 6.3 0.611 +9.356 1.9 0.00 3.9 1.2 0.36 3.3 IGR J16482-3036 252.040 -30.595 7.0 351.429 +9.231 3.0 0.88 3.4 0.0 0.00 0.0 1E 1743.1-2843 266.494 -28.762 0.0 0.189 +0.024 1.1 0.00 3.6 0.0 0.00 0.0 IGR J17451-3022 266.400 -30.325 6.8 358.812 -0.720 1.1 0.00 3.5 0.0 0.00 0.0 3A 1728-169 262.955 -16.898 6.9 8.578 +9.055 2.8 0.00 3.5 0.0 0.00 0.0 H 1702-429 256.538 -43.001 7.3 343.903 -1.282 7.6 2.31 3.3 0.0 0.00 0.0 IGR J17204-3554 260.163 -35.887 7.1 351.305 +0.626 1.6 0.00 3.4 0.0 0.00 0.0 Swift J181539.7-1833 273.968 -18.597 7.1 12.404 -0.862 2.4 0.00 3.4 0.0 0.00 0.0 XB 1832-330 278.910 -33.056 7.2 1.463 -11.382 2.1 0.00 3.3 0.0 0.00 0.0 IGR J17404-3655 265.074 -37.011 7.4 352.538 -3.291 1.5 0.00 3.2 0.0 0.00 0.0
JEM-X
JEM-X1 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 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 2.6 0.28 9.1 0.6 0.17 3.5 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 0.6 0.28 2.2 0.9 0.18 5.0 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.29 3.5 0.3 0.17 1.7 4U 1722-30 261.888 -30.802 356.320 +2.298 2.0 0.59 3.4 0.6 0.42 1.5 GX 1+4 263.009 -24.746 1.937 +4.795 1.5 1.07 1.4 2.6 0.72 3.6 GX 3+1 266.975 -26.575 2.280 +0.794 34.1 0.47 72.2 4.0 0.24 16.9 GX 354-0 262.989 -33.835 354.302 -0.150 9.5 1.15 8.3 4.3 0.97 4.4 GX 5-1 270.284 -25.097 5.062 -1.027 114.2 1.83 62.3 17.6 0.85 20.6 SLX 1737-282 265.163 -28.297 359.971 +1.264 1.3 0.30 4.3 0.3 0.18 1.8 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.9 0.28 6.9 0.4 0.17 2.2 NEW SOURCE 271.213 -25.592 5.044 -2.002 9.2 1.70 5.4 0.0 0.00 0.0 NEW SOURCE 267.914 -23.184 5.629 +1.804 12.7 2.42 5.2 0.0 0.00 0.0 NEW SOURCE 269.624 -24.496 5.285 -0.209 7.4 1.54 4.8 1.6 0.84 1.9 IGR J17497-2821 267.414 -28.358 0.953 -0.459 1.1 0.32 3.6 0.9 0.18 5.1