INTEGRAL Galactic bulge Monitoring
Revolution 0408: Observation start 2006-02-14T21:26 = MJD 53780.894
Total Observation GTI = 12111 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 1700-377 255.974 -37.851 0.8 347.744 +2.177 29.8 0.71 42.1 7.4 0.54 13.5 XTE J1817-330 274.422 -33.026 0.8 359.807 -7.992 17.2 0.42 40.7 6.8 0.33 20.3 GRS 1758-258 270.296 -25.742 0.9 4.507 -1.356 12.0 0.34 35.1 7.2 0.27 26.2 GX 5-1 270.281 -25.084 0.9 5.072 -1.019 12.5 0.37 33.5 0.0 0.00 0.0 GX 349+2 256.450 -36.421 0.9 349.112 +2.740 21.0 0.61 34.6 0.0 0.00 0.0 Ginga 1826-24 277.367 -23.793 0.9 9.276 -6.086 19.2 0.57 33.5 6.6 0.44 14.8 GX 1+4 263.005 -24.742 1.0 1.938 +4.800 11.4 0.37 31.1 0.0 0.00 0.0 1A 1742-294 266.505 -29.509 1.5 359.557 -0.372 5.7 0.29 19.4 2.7 0.25 10.8 GX 354-0 262.993 -33.816 1.8 354.319 -0.143 5.3 0.34 15.5 0.0 0.00 0.0 GX 17+2 274.022 -14.017 2.3 16.457 +1.273 26.6 2.27 11.7 0.0 0.00 0.0 H 1820-303 275.908 -30.395 2.8 2.754 -7.921 4.2 0.44 9.4 0.0 0.00 0.0 SLX 1735-269 264.550 -26.949 3.2 0.824 +2.440 2.5 0.31 8.0 1.5 0.26 5.5 4U 1722-30 261.857 -30.834 3.0 356.278 +2.302 3.0 0.34 8.7 1.8 0.28 6.4 3A 1822-371 276.463 -37.105 3.1 356.856 -11.303 4.9 0.59 8.3 2.3 0.47 4.9 IGR J17456-2901 266.415 -28.970 3.8 359.976 -0.025 1.9 0.28 6.7 0.0 0.00 0.0 SLX 1744-299_300 266.906 -30.018 3.5 359.302 -0.934 2.5 0.33 7.4 0.0 0.00 0.0 GX 3+1 266.976 -26.574 3.7 2.281 +0.794 2.1 0.30 6.9 0.0 0.00 0.0 GX 9+1 270.376 -20.536 3.7 9.067 +1.157 3.2 0.46 6.9 0.0 0.00 0.0 GX 13+1 273.662 -17.162 4.5 13.527 +0.079 4.5 0.81 5.5 0.0 0.00 0.0 IGR J17498-2921 267.500 -29.233 5.9 0.241 -0.973 1.2 0.30 4.2 0.0 0.00 0.0 SLX 1737-282 265.143 -28.361 5.1 359.908 +1.245 1.5 0.31 4.8 0.0 0.00 0.0 IGR J17541-2252 268.556 -22.857 6.2 6.210 +1.461 1.5 0.38 3.9 0.0 0.00 0.0 IGR J18027-1455 270.699 -14.935 5.9 14.098 +3.648 5.3 1.30 4.1 0.0 0.00 0.0 Oph Cluster 258.088 -23.285 5.8 0.629 +9.339 2.1 0.49 4.2 0.0 0.00 0.0 XTE J1710-281 257.661 -28.103 6.3 356.438 +6.861 1.7 0.43 3.9 0.0 0.00 0.0 GRS 1747-312 267.599 -31.249 6.2 358.552 -2.079 1.2 0.30 3.9 0.0 0.00 0.0 3A 1728-169 262.946 -17.033 6.0 8.458 +8.991 2.8 0.71 4.0 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 1.7 0.28 6.1 1.0 0.17 6.0 4U 1722-30 261.888 -30.802 356.320 +2.298 1.9 0.52 3.8 0.7 0.35 1.9 GRS 1747-312 267.690 -31.292 358.555 -2.168 1.9 0.36 5.3 0.5 0.22 2.5 GX 1+4 263.009 -24.746 1.937 +4.795 3.2 0.92 3.5 1.5 0.57 2.6 GX 3+1 266.988 -26.568 2.292 +0.788 21.4 0.44 48.4 2.2 0.22 9.6 GX 354-0 262.989 -33.835 354.302 -0.150 21.2 1.23 17.3 4.7 0.84 5.6 GX 5-1 270.281 -25.071 5.083 -1.012 131.9 2.07 63.7 13.8 0.89 15.5 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.1 0.37 3.1 0.0 0.00 0.0 SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.9 0.29 6.3 0.5 0.17 2.6 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.1 0.29 3.7 0.0 0.00 0.0 XTE J1739-285 264.975 -28.496 359.714 +1.298 5.7 0.30 19.1 0.7 0.17 3.9 NEW SOURCE 270.255 -24.400 5.654 -0.659 12.3 2.21 5.6 1.6 1.08 1.5 NEW SOURCE 272.200 -28.664 2.780 -4.259 5.6 1.11 5.0 0.7 0.67 1.1 NEW SOURCE 273.386 -27.066 4.690 -4.418 27.9 5.00 5.6 0.0 0.00 0.0