INTEGRAL Galactic bulge Monitoring
Revolution 1028: Observation start 2011-03-16T12:45 = MJD 55636.532
Total Observation GTI = 12075 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 +4.797 27.2 0.40 67.7 0.0 0.00 0.0 4U 1700-377 255.986 -37.848 0.6 347.751 +2.172 46.9 0.75 62.1 11.8 0.54 22.0 GX 354-0 262.990 -33.830 0.9 354.306 -0.148 13.8 0.41 33.4 4.9 0.32 15.5 GX 5-1 270.285 -25.071 1.1 5.084 -1.015 12.7 0.44 29.2 0.0 0.00 0.0 1E 1740.7-2942 265.981 -29.733 1.1 359.127 -0.101 9.5 0.33 29.0 5.8 0.26 22.8 Ginga 1826-24 277.372 -23.792 1.6 9.279 -6.089 13.6 0.77 17.6 5.8 0.55 10.4 IGR J17252-3616 261.291 -36.274 2.0 351.501 -0.344 6.2 0.46 13.6 1.7 0.34 4.9 GRS 1758-258 270.309 -25.736 1.8 4.517 -1.363 6.7 0.44 15.3 4.5 0.33 13.8 SAX J1806.5-2215 271.675 -22.249 2.6 8.168 -0.737 5.3 0.52 10.2 2.2 0.39 5.8 4U 1722-30 261.868 -30.798 3.1 356.314 +2.315 3.2 0.38 8.4 1.7 0.29 5.9 OAO 1657-415 255.169 -41.647 2.8 344.360 +0.345 11.2 1.21 9.3 0.0 0.00 0.0 IGR J17091-3624 257.294 -36.420 2.9 349.521 +2.197 5.2 0.58 8.9 0.0 0.00 0.0 3A 1822-371 276.517 -37.164 3.3 356.821 -11.368 5.4 0.68 7.9 0.0 0.00 0.0 GX 9+1 270.430 -20.563 3.5 9.068 +1.100 4.3 0.58 7.3 0.0 0.00 0.0 IGR J17177-3656 259.401 -36.928 4.2 350.100 +0.530 3.3 0.55 6.0 2.5 0.40 6.2 GX 17+2 274.027 -13.938 4.0 16.529 +1.307 46.7 7.37 6.3 0.0 0.00 0.0 AX J1749.2-2725 267.354 -27.315 5.1 1.820 +0.123 1.7 0.00 4.8 0.0 0.00 0.0 Oph Cluster 258.011 -23.291 5.4 0.583 +9.394 2.5 0.55 4.6 0.0 0.00 0.0 1A 1742-294 266.446 -29.543 0.0 359.500 -0.346 1.6 0.00 4.5 0.0 0.00 0.0 GX 349+2 256.461 -36.427 4.9 349.113 +2.730 3.1 0.62 5.0 0.0 0.00 0.0 H 1820-303 276.006 -30.289 0.0 2.888 -7.948 2.2 0.00 4.1 0.0 0.00 0.0 SAX J1712.6-3739 258.024 -37.591 6.8 348.922 +1.033 2.0 0.55 3.5 0.0 0.00 0.0 SLX 1744-299_300 266.735 -30.035 6.5 359.211 -0.816 1.3 0.00 3.7 0.0 0.00 0.0 PKS 1830-211 278.379 -21.003 6.5 12.202 -5.654 3.9 1.05 3.7 0.0 0.00 0.0 GX 3+1 267.013 -26.530 6.2 2.336 +0.789 1.4 0.35 3.9 0.0 0.00 0.0 XTE J1807-294 271.809 -29.323 0.0 2.035 -4.277 1.4 0.00 3.5 0.0 0.00 0.0 IGR J18048-1455 271.194 -14.983 5.9 14.290 +3.207 10.0 2.44 4.1 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 1742-294 266.522 -29.517 359.557 -0.389 10.8 0.23 46.3 1.8 0.14 13.2 1A 1743-288 266.757 -28.868 0.219 -0.228 4.7 0.25 19.2 0.3 0.14 2.1 1E 1740.7-2942 265.981 -29.748 359.114 -0.109 2.2 0.21 10.3 1.5 0.13 11.3 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.24 3.4 0.2 0.14 1.5 4U 1722-30 261.888 -30.802 356.320 +2.298 1.8 0.31 5.8 0.7 0.22 3.2 GX 1+4 263.009 -24.746 1.937 +4.795 1.3 0.97 1.3 3.2 0.71 4.5 GX 3+1 266.982 -26.566 2.291 +0.793 33.4 0.47 71.4 3.3 0.24 13.9 GX 354-0 262.989 -33.835 354.302 -0.150 7.2 0.47 15.4 2.7 0.35 7.6 GX 5-1 270.280 -25.077 5.077 -1.014 143.7 3.45 41.6 23.1 1.84 12.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.2 0.23 9.4 0.4 0.14 2.7 NEW SOURCE 272.030 -27.507 3.723 -3.571 10.7 2.09 5.1 0.0 0.00 0.0 NEW SOURCE 272.612 -28.504 3.094 -4.501 7.1 1.83 3.9 0.0 0.00 0.0 NEW SOURCE 270.421 -25.673 4.622 -1.420 6.1 1.68 3.6 0.0 0.00 0.0 NEW SOURCE 270.866 -27.107 3.570 -2.473 4.0 1.03 3.9 0.7 0.59 1.2 NEW SOURCE 271.649 -26.091 4.800 -2.588 13.1 2.85 4.6 2.1 1.57 1.4 NEW SOURCE 270.765 -26.924 3.685 -2.305 4.6 1.19 3.9 0.0 0.00 0.0