INTEGRAL Galactic bulge Monitoring
Revolution 0299: Observation start 2005-03-25T22:30 = MJD 53454.938
Total Observation GTI = 11928 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 5-1 270.289 -25.084 0.7 5.075 -1.024 16.5 0.31 52.6 1.0 0.00 4.0 IGR J17252-3616 261.297 -36.291 0.8 351.490 -0.358 16.9 0.40 42.3 1.5 0.32 4.8 GRS 1758-258 270.306 -25.740 0.9 4.513 -1.363 12.2 0.35 35.3 7.9 0.28 28.6 GX 354-0 263.003 -33.829 1.0 354.313 -0.156 10.4 0.35 30.0 1.4 0.28 5.2 Ginga 1826-24 277.362 -23.788 1.1 9.278 -6.079 16.6 0.58 28.7 6.4 0.44 14.5 1E 1740.7-2942 265.971 -29.748 1.2 359.110 -0.102 8.1 0.32 25.0 4.3 0.27 16.2 OAO 1657-415 255.181 -41.661 1.2 344.355 +0.329 33.3 1.38 24.2 6.7 1.02 6.6 IGR J17098-3628 257.443 -36.470 1.3 349.551 +2.071 12.2 0.55 22.4 5.2 0.42 12.4 GX 349+2 256.449 -36.412 2.2 349.119 +2.747 6.6 0.53 12.5 0.0 0.00 0.0 GX 1+4 263.023 -24.759 2.0 1.933 +4.777 4.3 0.32 13.4 0.0 0.00 0.0 4U 1722-30 261.886 -30.776 2.3 356.340 +2.314 3.6 0.31 11.8 0.9 0.25 3.8 H 1820-303 275.908 -30.361 2.3 2.784 -7.905 5.7 0.50 11.4 0.0 0.00 0.0 3A 1822-371 276.423 -37.075 2.8 356.870 -11.262 6.4 0.67 9.5 0.0 0.00 0.0 GX 9+1 270.366 -20.486 2.9 9.106 +1.190 4.2 0.47 8.9 0.0 0.00 0.0 SLX 1735-269 264.564 -27.026 2.8 0.765 +2.388 2.7 0.29 9.3 0.0 0.00 0.0 GX 3+1 266.940 -26.532 3.1 2.301 +0.843 2.6 0.31 8.4 0.0 0.00 0.0 XTE J1743-363 265.688 -36.364 4.1 353.349 -3.369 2.3 0.37 6.1 1.4 0.30 4.6 GX 13+1 273.602 -17.157 3.9 13.504 +0.131 5.2 0.80 6.5 0.0 0.00 0.0 SLX 1744-299_300 266.860 -30.078 6.1 359.230 -0.931 1.3 0.34 4.0 0.0 0.00 0.0 1A 1743-288 266.674 -28.812 6.2 0.228 -0.137 1.1 0.28 3.9 0.0 0.00 0.0 AX J1749.1-2733 267.278 -27.537 5.0 1.595 +0.067 1.5 0.31 5.0 0.0 0.00 0.0 IGR J17191-2821 259.710 -28.260 5.5 357.357 +5.295 1.5 0.34 4.4 0.0 0.00 0.0 IGR J17473-2721 266.860 -27.340 5.2 1.572 +0.486 1.4 0.30 4.8 0.0 0.00 0.0 Oph Cluster 258.011 -23.412 5.9 0.483 +9.324 1.9 0.00 4.1 0.0 0.00 0.0 SLX 1737-282 265.212 -28.245 6.0 0.038 +1.254 1.3 0.32 4.1 0.0 0.00 0.0 GX 17+2 274.026 -14.006 5.3 16.468 +1.275 12.2 2.63 4.6 0.0 0.00 0.0 IGR J17195-4100 259.902 -40.986 6.5 347.003 -2.122 3.0 0.80 3.7 0.0 0.00 0.0 IGR J17088-4008 257.175 -40.048 6.3 346.552 +0.108 3.2 0.82 3.9 0.0 0.00 0.0 IGR J18249-3243 276.305 -32.668 5.7 0.852 -9.242 2.0 0.46 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 1742-294 266.500 -29.524 359.542 -0.377 1.9 0.22 8.9 0.6 0.13 4.7 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.21 9.7 0.0 0.00 0.0 4U 1722-30 261.888 -30.802 356.320 +2.298 1.9 0.37 5.3 0.6 0.26 2.2 GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 0.9 0.22 4.1 0.0 0.00 0.0 GX 3+1 266.985 -26.566 2.292 +0.791 19.6 0.35 56.1 2.1 0.18 11.6 GX 354-0 262.989 -33.835 354.302 -0.150 8.5 0.76 11.1 2.3 0.58 4.0 GX 5-1 270.283 -25.088 5.069 -1.022 120.5 1.73 69.8 15.4 0.77 20.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.0 0.23 12.9 0.4 0.14 3.0 NEW SOURCE 270.168 -24.958 5.130 -0.867 4.9 1.39 3.6 1.8 0.68 2.6