INTEGRAL Galactic bulge Monitoring
Revolution 0288: Observation start 2005-02-21T08:15 = MJD 53422.344
Total Observation GTI = 9814 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 1700-377 255.991 -37.845 0.5 347.756 +2.170 63.0 0.80 78.4 16.5 0.61 27.1 1E 1740.7-2942 265.971 -29.744 1.0 359.113 -0.100 9.6 0.30 32.5 6.0 0.25 24.5 GRS 1758-258 270.300 -25.744 1.1 4.507 -1.360 11.5 0.40 29.0 8.4 0.32 26.6 Ginga 1826-24 277.366 -23.801 1.2 9.268 -6.088 15.1 0.62 24.4 4.1 0.48 8.6 GX 354-0 262.991 -33.837 1.2 354.301 -0.153 9.0 0.36 24.7 0.0 0.00 0.0 GX 349+2 256.435 -36.420 1.6 349.106 +2.751 11.5 0.66 17.5 0.0 0.00 0.0 H 1820-303 275.931 -30.358 1.8 2.796 -7.922 7.9 0.52 15.2 0.0 0.00 0.0 GX 1+4 263.005 -24.747 1.8 1.934 +4.797 5.5 0.37 15.1 0.0 0.00 0.0 OAO 1657-415 255.206 -41.651 2.0 344.374 +0.321 28.0 2.00 14.0 6.2 1.38 4.5 4U 1722-30 261.915 -30.841 2.3 356.300 +2.257 4.3 0.37 11.8 1.3 0.30 4.4 GX 17+2 274.020 -13.995 3.1 16.475 +1.285 17.3 2.06 8.4 0.0 0.00 0.0 GX 9+1 270.392 -20.537 3.0 9.073 +1.143 4.2 0.49 8.7 0.0 0.00 0.0 3A 1822-371 276.473 -37.094 3.2 356.871 -11.306 6.4 0.78 8.2 0.0 0.00 0.0 GX 3+1 266.947 -26.518 3.3 2.316 +0.845 2.8 0.35 7.9 0.0 0.00 0.0 1E 1742.8-2853 266.462 -28.948 3.4 0.016 -0.049 2.1 0.29 7.4 0.0 0.00 0.0 SLX 1735-269 264.574 -27.000 3.7 0.792 +2.395 2.4 0.34 6.9 0.0 0.00 0.0 SLX 1744-299_300 266.924 -29.982 3.9 359.341 -0.929 2.0 0.30 6.5 0.0 0.00 0.0 GX 5-1 270.268 -25.061 4.7 5.086 -0.997 2.1 0.39 5.3 0.0 0.00 0.0 1A 1742-294 266.578 -29.486 4.2 359.609 -0.415 1.8 0.29 6.0 0.0 0.00 0.0 IGR J17544-2619 268.556 -26.374 4.9 3.177 -0.319 1.9 0.38 5.0 0.0 0.00 0.0 GRO J1655-40 253.530 -39.841 4.3 345.000 +2.441 6.3 1.08 5.8 0.0 0.00 0.0 XB 1832-330 278.911 -32.945 5.0 1.566 -11.335 3.4 0.68 4.9 0.0 0.00 0.0 3A 1728-169 262.954 -16.969 4.7 8.517 +9.018 3.6 0.68 5.3 0.0 0.00 0.0 1H 1746-370 267.624 -37.049 0.0 353.562 -5.053 2.1 0.00 4.0 0.0 0.00 0.0 H 1702-429 256.529 -43.057 6.3 343.854 -1.311 11.3 0.00 3.9 0.0 0.00 0.0 IGR J17331-2406 263.266 -24.016 5.9 2.680 +4.993 1.5 0.35 4.2 0.0 0.00 0.0 IGR J17597-2201 269.846 -21.982 6.0 7.566 +0.868 1.6 0.40 4.1 0.0 0.00 0.0 Swift J175648.6-2544 269.195 -25.812 0.0 3.952 -0.531 1.4 0.00 3.6 0.0 0.00 0.0 SLX 1737-282 265.231 -28.238 7.6 0.053 +1.244 0.9 0.30 3.1 0.0 0.00 0.0 IGR J17252-3616 261.344 -36.238 0.0 351.555 -0.360 1.6 0.00 3.4 0.0 0.00 0.0 Swift J1753.7-2544 268.442 -25.860 6.9 3.568 +0.030 1.4 0.39 3.5 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 0.22 10.8 0.6 0.13 4.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.4 0.21 6.6 1.1 0.13 8.9 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.22 4.4 0.2 0.13 1.3 4U 1722-30 261.888 -30.802 356.320 +2.298 1.7 0.37 4.5 0.6 0.26 2.4 GX 3+1 266.984 -26.563 2.294 +0.794 24.5 0.36 68.4 2.8 0.18 15.7 GX 354-0 262.994 -33.829 354.309 -0.150 17.6 0.89 19.7 4.4 0.63 7.0 GX 5-1 270.284 -25.072 5.084 -1.015 104.7 1.69 61.9 6.2 0.72 8.6 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.4 0.23 6.2 0.3 0.13 2.6 CONFUSED ID 270.284 -25.072 5.083 -1.015 104.6 1.69 61.9 6.2 0.72 8.7 NEW SOURCE 266.161 -23.494 4.532 +3.024 5.8 0.96 6.0 0.6 0.55 1.1 NEW SOURCE 270.196 -25.788 4.421 -1.301 4.6 0.88 5.3 0.0 0.00 0.0 NEW SOURCE 268.893 -23.381 5.915 +0.929 9.0 1.82 5.0 1.7 0.97 1.7 CONFUSED ID 270.279 -25.001 5.143 -0.976 28.9 1.47 19.6 1.6 0.69 2.3 NEW SOURCE 270.466 -24.849 5.359 -1.048 7.5 1.56 4.8 0.9 0.75 1.2 MULTIPLE ID 266.342 -28.985 359.930 +0.022 1.1 0.22 5.1 0.0 0.00 0.0