INTEGRAL Galactic bulge Monitoring
Revolution 0663: Observation start 2008-03-18T18:01 = MJD 54543.751
Total Observation GTI = 12019 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 J1750-27 267.297 -26.643 0.5 2.370 +0.513 30.4 0.36 85.1 1.3 0.00 4.3 4U 1700-377 255.991 -37.841 0.8 347.759 +2.173 36.7 0.95 38.5 9.1 0.72 12.5 Ginga 1826-24 277.366 -23.799 1.0 9.270 -6.088 18.9 0.61 30.9 7.0 0.46 15.0 H 1820-303 275.916 -30.348 1.1 2.799 -7.906 14.1 0.51 27.7 0.0 0.00 0.0 4U 1722-30 261.878 -30.799 1.4 356.318 +2.307 8.3 0.39 21.5 3.1 0.31 10.2 GX 5-1 270.279 -25.087 1.5 5.068 -1.018 7.1 0.36 19.4 0.0 0.00 0.0 GX 354-0 262.971 -33.851 1.6 354.280 -0.146 7.7 0.45 17.2 1.8 0.36 4.9 GRS 1758-258 270.313 -25.740 2.0 4.516 -1.368 5.3 0.39 13.4 3.2 0.31 10.1 GX 3+1 266.929 -26.582 0.0 2.253 +0.826 3.7 0.00 10.5 0.0 0.00 0.0 1E 1740.7-2942 265.976 -29.743 2.4 359.117 -0.102 4.3 0.38 11.3 1.8 0.31 5.9 3A 1822-371 276.451 -37.141 2.7 356.819 -11.311 6.5 0.67 9.7 0.0 0.00 0.0 SAX J1750.8-2900 267.606 -29.025 2.6 0.467 -0.945 3.6 0.35 10.2 0.0 0.00 0.0 XTE J1810-189 272.567 -19.081 2.7 11.343 +0.069 5.7 0.60 9.6 3.9 0.47 8.3 GX 9+1 270.362 -20.535 2.7 9.061 +1.169 4.2 0.43 9.7 0.0 0.00 0.0 GX 349+2 256.436 -36.419 3.0 349.107 +2.751 6.7 0.78 8.6 0.0 0.00 0.0 GX 1+4 263.050 -24.748 3.0 1.956 +4.762 3.1 0.36 8.8 0.0 0.00 0.0 3A 1728-169 262.902 -16.959 4.4 8.499 +9.066 4.1 0.72 5.7 0.0 0.00 0.0 MXB 1730-335 263.265 -33.365 4.3 354.821 -0.086 2.6 0.44 5.8 0.0 0.00 0.0 SLX 1735-269 264.556 -26.964 4.3 0.815 +2.428 2.1 0.36 5.8 1.2 0.30 3.9 1E 1742.9-2849 266.479 -28.859 4.7 0.099 -0.015 1.7 0.33 5.3 0.0 0.00 0.0 IGR J17473-2721 266.835 -27.404 5.1 1.506 +0.472 1.5 0.00 4.8 0.0 0.00 0.0 XB 1832-330 278.975 -33.015 4.8 1.524 -11.413 3.4 0.65 5.2 0.0 0.00 0.0 1RXS J170849.0-40091 257.170 -40.177 5.5 346.446 +0.035 5.7 0.00 4.5 0.0 0.00 0.0 1A 1742-294 266.545 -29.472 5.2 359.606 -0.383 1.7 0.36 4.8 0.0 0.00 0.0 Swift J1749.4-2807 267.393 -28.145 0.0 1.126 -0.333 1.3 0.00 4.2 0.0 0.00 0.0 SLX 1744-299_300 266.860 -29.929 5.8 359.357 -0.854 1.6 0.37 4.2 0.0 0.00 0.0 GX 17+2 273.960 -14.017 5.5 16.428 +1.326 8.1 1.82 4.5 0.0 0.00 0.0 IGR J17559-2612 268.945 -26.159 0.0 3.538 -0.512 1.6 0.00 4.0 0.0 0.00 0.0 IGR J17464-3213 266.656 -32.215 5.6 357.311 -1.890 1.5 0.34 4.3 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 2.2 0.37 5.9 0.6 0.22 2.6 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.4 0.39 3.5 0.4 0.24 1.7 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.1 0.36 3.1 0.4 0.21 1.8 4U 1722-30 261.888 -30.802 356.320 +2.298 3.6 1.15 3.1 2.0 0.89 2.3 GRO J1750-27 267.305 -26.645 2.372 +0.505 8.7 0.45 19.4 7.8 0.26 30.4 GRS 1747-312 267.690 -31.292 358.555 -2.168 2.0 0.54 3.7 0.6 0.33 1.9 GX 3+1 266.982 -26.562 2.294 +0.796 50.2 0.48 103.8 5.6 0.25 22.6 GX 5-1 270.291 -25.076 5.083 -1.023 128.2 1.34 95.4 12.7 0.61 20.9 SAX J1750.8-2900 267.602 -29.031 0.460 -0.946 13.1 0.40 33.0 2.3 0.23 10.2 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.7 0.40 4.4 0.4 0.24 1.6 NEW SOURCE 267.497 -22.271 6.217 +2.601 12.8 2.41 5.3 0.0 0.00 0.0 NEW SOURCE 273.657 -28.072 3.914 -5.105 11.3 2.20 5.2 0.0 0.00 0.0 NEW SOURCE 269.460 -30.551 359.963 -3.105 2.4 0.56 4.3 0.5 0.34 1.4 NEW SOURCE 266.396 -21.491 6.360 +3.878 19.1 4.06 4.7 2.8 2.69 1.0 NEW SOURCE 271.148 -24.080 6.334 -1.210 9.6 2.37 4.0 0.0 0.00 0.0 NEW SOURCE 272.792 -25.077 6.187 -3.001 14.8 3.53 4.2 2.7 1.78 1.5 NEW SOURCE 267.954 -27.526 1.912 -0.443 0.7 0.41 1.7 0.7 0.22 3.2