INTEGRAL Galactic bulge Monitoring
Revolution 0354: Observation start 2005-09-07T03:04 = MJD 53620.129
Total Observation GTI = 12130 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 1700-377 255.985 -37.843 0.5 347.754 +2.175 60.3 0.71 84.9 13.9 0.53 26.2 GRS 1758-258 270.305 -25.744 0.8 4.508 -1.364 12.4 0.31 40.0 7.2 0.25 29.0 Ginga 1826-24 277.360 -23.793 1.0 9.273 -6.080 18.9 0.58 32.6 6.5 0.45 14.6 1E 1740.7-2942 265.978 -29.748 1.2 359.113 -0.107 7.6 0.29 26.1 4.3 0.23 18.5 GX 1+4 263.015 -24.740 1.2 1.945 +4.793 9.0 0.35 25.9 0.0 0.00 0.0 GX 349+2 256.443 -36.419 1.5 349.110 +2.746 12.3 0.62 19.9 0.0 0.00 0.0 H 1820-303 275.919 -30.365 1.6 2.784 -7.915 8.2 0.46 17.8 0.0 0.00 0.0 IGR J17454-2919 266.345 -29.392 1.8 359.583 -0.193 4.1 0.27 15.2 0.0 0.00 0.0 GX 5-1 270.285 -25.097 2.0 5.062 -1.028 4.3 0.32 13.5 0.0 0.00 0.0 GX 354-0 262.972 -33.851 2.0 354.281 -0.147 4.7 0.34 13.7 1.0 0.27 3.9 GX 17+2 273.996 -14.033 2.2 16.430 +1.288 33.6 2.75 12.2 0.0 0.00 0.0 4U 1722-30 261.829 -30.778 2.5 356.311 +2.354 3.2 0.31 10.6 1.1 0.24 4.7 GX 9+1 270.410 -20.508 3.0 9.107 +1.143 4.2 0.48 8.7 0.0 0.00 0.0 GX 3+1 267.013 -26.563 2.7 2.308 +0.771 2.8 0.28 9.7 0.0 0.00 0.0 IGR J17464-3213 266.545 -32.237 2.8 357.243 -1.820 2.9 0.30 9.5 1.8 0.25 7.4 SLX 1735-269 264.590 -26.997 3.2 0.802 +2.385 2.3 0.29 8.1 1.6 0.23 7.0 SLX 1737-282 265.122 -28.313 4.3 359.938 +1.286 1.6 0.27 5.9 0.0 0.00 0.0 3A 1822-371 276.395 -37.019 4.7 356.911 -11.217 3.3 0.62 5.3 0.0 0.00 0.0 V2400 Oph 258.075 -24.230 4.8 359.839 +8.806 2.3 0.45 5.2 0.0 0.00 0.0 GRS 1747-312 267.757 -31.261 7.8 358.612 -2.202 0.9 0.29 3.1 0.0 0.00 0.0 3A 1728-169 262.923 -16.954 4.4 8.514 +9.051 4.2 0.74 5.7 0.0 0.00 0.0 SLX 1744-299_300 266.768 -30.050 4.7 359.213 -0.849 1.4 0.28 5.2 0.0 0.00 0.0 1E 1742.8-2853 266.401 -28.922 0.0 0.011 +0.011 1.3 0.00 4.9 0.0 0.00 0.0 IGR J17361-4441 264.096 -44.780 4.6 345.528 -6.776 20.3 3.78 5.4 0.0 0.00 0.0 IGR J17488-3253 267.141 -32.917 4.8 356.921 -2.602 1.6 0.31 5.1 0.0 0.00 0.0 IGR J18027-2016 270.642 -20.215 0.0 9.469 +1.099 2.1 0.00 4.1 0.0 0.00 0.0 IGR J17252-3616 261.277 -36.276 6.3 351.493 -0.337 1.8 0.47 3.9 0.0 0.00 0.0 AX J1754.2-2754 268.693 -27.941 6.1 1.886 -1.216 1.1 0.28 4.0 0.0 0.00 0.0 IGR J17475-2822 266.775 -28.427 0.0 0.603 -0.013 1.0 0.00 3.7 0.0 0.00 0.0 IGR J18048-1455 271.258 -14.926 6.6 14.370 +3.181 4.7 1.27 3.7 0.0 0.00 0.0 GRO J1744-28 266.025 -28.756 0.0 359.979 +0.378 1.0 0.00 3.6 0.0 0.00 0.0 XTE J1817-330 274.379 -32.925 7.5 359.881 -7.913 1.3 0.41 3.2 1.2 0.00 3.7 GX 13+1 273.618 -17.108 7.1 13.553 +0.141 2.8 0.00 3.4 0.0 0.00 0.0 Swift J165534.1-4426 253.894 -44.502 5.8 341.545 -0.700 39.4 9.27 4.2 0.0 0.00 0.0 XB 1733-30 263.922 -30.379 7.1 357.633 +1.064 0.9 0.00 3.4 0.0 0.00 0.0 IGR J16482-3036 252.107 -30.556 3.9 351.498 +9.211 4.8 0.73 6.5 0.0 0.00 0.0 NEW SOURCE 266.684 -29.497 0.0 359.648 -0.500 1.7 0.00 6.4 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 2.4 0.25 9.3 0.7 0.15 4.9 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.9 0.26 7.3 1.2 0.16 7.9 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.26 3.3 0.2 0.15 1.6 4U 1722-30 261.888 -30.802 356.320 +2.298 3.1 0.56 5.5 1.0 0.40 2.5 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.5 0.31 4.8 0.6 0.19 3.2 GRS 1758-258 270.303 -25.741 4.511 -1.361 2.9 0.90 3.2 1.0 0.44 2.2 GX 1+4 263.009 -24.746 1.937 +4.795 0.0 0.00 0.0 2.3 0.61 3.8 GX 3+1 266.995 -26.565 2.298 +0.784 25.4 0.40 64.2 2.6 0.20 13.0 GX 354-0 262.990 -33.841 354.297 -0.154 20.1 1.24 16.2 4.0 0.88 4.6 GX 5-1 270.283 -25.074 5.081 -1.015 99.9 1.55 64.4 7.3 0.64 11.5 IGR J17464-3213 266.567 -32.229 357.260 -1.832 3.4 0.37 9.3 0.9 0.24 4.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.1 0.33 3.4 0.5 0.20 2.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.26 6.9 0.5 0.16 3.2 NEW SOURCE 271.334 -26.995 3.872 -2.782 3.6 0.82 4.4 0.0 0.00 0.0 NEW SOURCE 271.041 -24.435 5.977 -1.299 10.0 2.64 3.8 0.0 0.00 0.0 NEW SOURCE 267.677 -25.023 3.936 +1.050 2.6 0.65 4.0 0.0 0.00 0.0 KS 1741-293 266.221 -29.346 359.566 -0.076 1.0 0.25 4.0 0.5 0.15 3.3