INTEGRAL Galactic bulge Monitoring
Revolution 0410: Observation start 2006-02-20T20:52 = MJD 53786.87
Total Observation GTI = 11812 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+4 263.006 -24.741 0.9 1.939 +4.800 12.4 0.33 37.8 0.0 0.00 0.0 GRS 1758-258 270.297 -25.748 1.0 4.502 -1.360 10.4 0.34 30.6 5.9 0.28 21.5 XTE J1817-330 274.433 -33.018 1.0 359.818 -7.997 13.2 0.42 31.2 6.0 0.34 17.8 GX 349+2 256.426 -36.421 1.1 349.100 +2.756 17.0 0.58 29.4 0.0 0.00 0.0 Ginga 1826-24 277.365 -23.792 1.1 9.276 -6.083 17.3 0.61 28.6 6.9 0.47 14.7 GX 5-1 270.288 -25.074 1.2 5.084 -1.019 8.3 0.32 25.6 0.0 0.00 0.0 1A 1742-294 266.518 -29.511 1.3 359.560 -0.383 6.6 0.28 23.4 1.9 0.24 8.2 OAO 1657-415 255.204 -41.654 1.2 344.371 +0.320 37.5 1.54 24.3 6.9 1.14 6.1 GX 354-0 262.997 -33.847 1.2 354.296 -0.163 8.2 0.34 24.4 0.0 0.00 0.0 4U 1700-377 255.995 -37.848 1.4 347.755 +2.166 13.4 0.65 20.7 2.3 0.50 4.7 H 1820-303 275.925 -30.372 1.5 2.781 -7.923 8.8 0.47 18.6 0.0 0.00 0.0 3A 1822-371 276.460 -37.108 2.7 356.853 -11.302 6.0 0.61 10.0 0.0 0.00 0.0 IGR J17252-3616 261.314 -36.278 2.5 351.509 -0.363 4.8 0.46 10.5 0.0 0.00 0.0 GX 17+2 273.971 -14.043 2.8 16.410 +1.304 23.0 2.46 9.3 0.0 0.00 0.0 SLX 1735-269 264.586 -26.984 3.2 0.811 +2.395 2.9 0.36 8.1 0.0 0.00 0.0 4U 1722-30 261.890 -30.785 3.2 356.335 +2.306 2.8 0.35 8.1 0.0 0.00 0.0 SLX 1744-299_300 266.822 -29.974 3.7 359.302 -0.850 2.1 0.30 6.9 0.0 0.00 0.0 GX 3+1 266.999 -26.544 3.5 2.318 +0.792 2.6 0.35 7.3 0.0 0.00 0.0 3A 1728-169 262.905 -16.963 4.1 8.497 +9.061 4.3 0.70 6.1 0.0 0.00 0.0 GX 13+1 273.550 -17.154 4.2 13.482 +0.176 4.9 0.81 6.0 0.0 0.00 0.0 Swift J174535.5-2901 266.401 -29.086 0.0 359.870 -0.075 1.2 0.00 4.2 0.0 0.00 0.0 1E 1743.1-2843 266.561 -28.707 5.7 0.267 +0.002 1.2 0.28 4.3 0.0 0.00 0.0 GX 9+1 270.413 -20.596 6.0 9.032 +1.097 1.8 0.45 4.0 0.0 0.00 0.0 GRS 1747-312 267.555 -31.301 6.5 358.489 -2.074 1.3 0.00 3.7 0.0 0.00 0.0 Oph Cluster 258.187 -23.420 6.5 0.570 +9.188 1.8 0.49 3.7 0.0 0.00 0.0 SLX 1737-282 265.197 -28.258 8.9 0.020 +1.258 0.8 0.30 2.6 0.0 0.00 0.0 V2400 Oph 258.259 -24.187 0.0 359.972 +8.693 1.7 0.00 3.6 0.0 0.00 0.0 IGR J17464-2811 266.868 -28.262 6.9 0.787 +0.003 1.0 0.00 3.5 0.0 0.00 0.0 XTE J1743-363 265.836 -36.336 7.0 353.436 -3.456 1.4 0.42 3.4 0.0 0.00 0.0 IGR J16316-4028 247.791 -40.416 7.1 341.680 +5.376 16.7 0.00 3.4 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 2.1 0.29 7.3 1.0 0.17 5.6 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.9 0.36 5.4 0.0 0.00 0.0 GX 3+1 266.986 -26.569 2.291 +0.789 26.2 0.45 58.0 3.1 0.23 13.2 GX 354-0 262.989 -33.830 354.306 -0.147 33.5 1.31 25.6 6.2 0.86 7.2 GX 5-1 270.295 -25.072 5.088 -1.023 107.1 1.88 56.9 10.4 0.82 12.7 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.2 0.38 3.2 0.0 0.00 0.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.7 0.30 5.8 0.3 0.18 2.0 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.1 0.30 3.7 0.2 0.17 1.3 XTE J1739-285 264.978 -28.499 359.714 +1.295 6.8 0.30 22.3 0.7 0.17 3.9 CONFUSED ID 270.282 -25.074 5.081 -1.014 111.2 1.88 59.1 11.1 0.82 13.6 NEW SOURCE 269.541 -23.558 6.060 +0.326 12.9 2.47 5.2 1.7 1.43 1.2 CONFUSED ID 270.316 -25.000 5.160 -1.005 27.5 1.74 15.9 2.1 0.81 2.5 NEW SOURCE 266.999 -22.422 5.851 +2.919 16.1 2.97 5.4 0.0 0.00 0.0