INTEGRAL Galactic bulge Monitoring
Revolution 0289: Observation start 2005-02-24T01:17 = MJD 53425.054
Total Observation GTI = 12059 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 1700-377 255.995 -37.850 0.5 347.753 +2.165 55.8 0.62 90.0 14.6 0.47 30.9 GRS 1758-258 270.297 -25.744 0.9 4.505 -1.358 11.7 0.34 34.9 8.6 0.27 31.7 GX 5-1 270.275 -25.087 0.9 5.067 -1.015 11.6 0.35 33.4 0.0 0.00 0.0 1E 1740.7-2942 265.978 -29.746 1.0 359.115 -0.106 9.0 0.27 33.1 6.1 0.23 26.1 Ginga 1826-24 277.364 -23.794 1.4 9.274 -6.084 12.9 0.60 21.5 4.7 0.47 10.0 GX 349+2 256.415 -36.415 1.6 349.100 +2.766 10.5 0.58 17.9 0.0 0.00 0.0 GX 354-0 262.977 -33.832 1.5 354.299 -0.140 6.8 0.37 18.4 0.0 0.00 0.0 H 1820-303 275.921 -30.365 1.7 2.785 -7.917 7.4 0.46 16.0 0.0 0.00 0.0 4U 1722-30 261.916 -30.789 2.4 356.344 +2.286 3.7 0.33 11.2 1.7 0.27 6.3 3A 1822-371 276.436 -37.106 2.4 356.846 -11.285 6.6 0.58 11.4 0.0 0.00 0.0 1A 1742-294 266.481 -29.455 2.8 359.592 -0.326 2.5 0.26 9.3 0.0 0.00 0.0 GX 17+2 274.052 -14.061 2.6 16.432 +1.226 24.9 2.49 10.0 0.0 0.00 0.0 GX 13+1 273.664 -17.153 2.9 13.535 +0.081 7.3 0.80 9.1 0.0 0.00 0.0 SLX 1735-269 264.570 -26.958 2.8 0.826 +2.421 2.7 0.29 9.4 1.2 0.25 4.9 GX 9+1 270.384 -20.551 3.2 0.000 +0.000 3.4 0.42 8.0 0.0 0.00 0.0 GX 1+4 262.996 -24.739 3.5 1.936 +4.809 2.7 0.37 7.3 0.0 0.00 0.0 GX 3+1 267.013 -26.568 3.6 2.304 +0.769 2.1 0.29 7.1 0.0 0.00 0.0 GRO J1655-40 253.478 -39.881 5.1 344.943 +2.447 5.6 1.15 4.9 4.4 0.80 5.5 3A 1728-169 262.916 -16.935 5.3 8.526 +9.066 3.3 0.71 4.7 0.0 0.00 0.0 1E 1743.1-2843 266.563 -28.718 0.0 0.258 -0.005 1.4 0.00 5.3 0.0 0.00 0.0 OAO 1657-415 255.188 -41.662 4.4 344.357 +0.324 8.9 1.57 5.7 0.0 0.00 0.0 IGR J17252-3616 261.345 -36.236 0.0 351.557 -0.359 2.0 0.00 4.8 0.0 0.00 0.0 SAX J1712.6-3739 258.170 -37.631 5.1 348.957 +0.917 2.9 0.60 4.8 0.0 0.00 0.0 PKS 1830-211 278.469 -21.142 4.9 12.116 -5.792 3.9 0.77 5.1 0.0 0.00 0.0 1RXS J165443.5-19162 262.569 -19.391 6.1 6.249 +8.032 1.9 0.00 4.0 0.0 0.00 0.0 IGR J17448-3232 266.094 -32.582 6.4 356.751 -1.675 1.3 0.00 3.8 0.0 0.00 0.0 Swift J174535.5-2901 266.376 -29.130 0.0 359.821 -0.080 1.0 0.00 3.8 0.0 0.00 0.0 IGR J18135-1751 273.439 -17.774 6.5 12.888 -0.027 2.7 0.00 3.7 0.0 0.00 0.0 V1223 Sgr 283.844 -31.124 6.7 5.025 -14.406 8.5 2.35 3.6 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 1.8 0.22 8.4 0.5 0.13 4.1 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.0 0.21 9.3 1.0 0.13 7.6 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.7 0.22 3.4 0.3 0.13 2.4 4U 1722-30 261.888 -30.802 356.320 +2.298 2.2 0.39 5.8 0.8 0.25 3.1 GRS 1758-258 270.303 -25.741 4.511 -1.361 4.3 0.99 4.3 1.2 0.49 2.4 GX 3+1 266.984 -26.554 2.302 +0.798 21.2 0.35 59.8 2.3 0.17 13.3 GX 354-0 262.994 -33.828 354.310 -0.150 21.8 0.93 23.4 4.6 0.64 7.2 GX 5-1 270.281 -25.044 5.107 -0.999 93.1 1.71 54.5 7.6 0.76 9.9 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.8 0.23 8.0 0.3 0.13 2.4 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.7 0.22 3.0 0.0 0.00 0.0 XTE J1739-285 264.975 -28.496 359.714 +1.298 0.7 0.22 3.1 0.0 0.00 0.0 CONFUSED ID 270.283 -25.071 5.084 -1.014 116.7 1.76 66.2 11.0 0.79 13.8 CONFUSED ID 270.312 -24.985 5.171 -0.994 20.4 1.54 13.2 1.2 0.75 1.6