INTEGRAL Galactic bulge Monitoring
Revolution 0287: Observation start 2005-02-18T07:12 = MJD 53419.301
Total Observation GTI = 11504 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 1700-377 255.987 -37.853 0.4 347.747 +2.168 92.2 0.72 128.5 22.9 0.52 43.6 GX 354-0 262.989 -33.839 0.7 354.299 -0.152 14.9 0.32 46.8 3.1 0.25 12.2 GRS 1758-258 270.287 -25.743 0.9 4.502 -1.350 12.1 0.36 33.6 7.8 0.28 27.8 1E 1740.7-2942 265.970 -29.739 1.0 359.117 -0.096 9.8 0.31 31.6 5.8 0.25 22.9 Ginga 1826-24 277.370 -23.791 1.2 9.278 -6.087 14.0 0.54 25.8 6.4 0.41 15.5 GX 5-1 270.272 -25.065 1.4 5.084 -1.002 7.9 0.37 21.3 0.0 0.00 0.0 H 1820-303 275.913 -30.348 1.6 2.797 -7.903 8.2 0.45 18.2 0.0 0.00 0.0 OAO 1657-415 255.210 -41.654 1.6 344.374 +0.317 22.8 1.33 17.1 5.1 0.92 5.5 GX 349+2 256.425 -36.411 1.7 349.108 +2.763 9.0 0.55 16.5 0.0 0.00 0.0 GX 17+2 273.986 -14.025 1.9 16.433 +1.299 32.5 2.27 14.3 0.0 0.00 0.0 4U 1722-30 261.876 -30.782 2.1 356.331 +2.318 4.1 0.31 13.2 1.5 0.24 6.3 GX 9+1 270.373 -20.522 2.0 9.078 +1.167 5.9 0.45 13.3 0.0 0.00 0.0 3A 1822-371 276.416 -37.095 3.1 356.849 -11.266 5.8 0.69 8.4 0.0 0.00 0.0 SLX 1735-269 264.519 -26.964 3.2 0.797 +2.456 2.4 0.30 8.1 1.2 0.24 4.9 GX 3+1 266.964 -26.563 3.5 2.285 +0.809 2.1 0.29 7.4 0.0 0.00 0.0 SLX 1744-299_300 266.814 -30.042 4.5 359.241 -0.879 1.6 0.29 5.5 0.0 0.00 0.0 IGR J17252-3616 261.298 -36.263 4.7 351.514 -0.343 2.3 0.43 5.3 0.0 0.00 0.0 V2400 Oph 258.208 -24.199 4.7 359.935 +8.725 2.3 0.43 5.3 0.0 0.00 0.0 SAX J1712.6-3739 258.151 -37.660 5.3 348.925 +0.912 2.7 0.57 4.7 0.0 0.00 0.0 GRS 1734-292 264.355 -29.134 5.6 358.884 +1.417 1.5 0.35 4.4 0.0 0.00 0.0 IGR J17473-2721 266.757 -27.332 5.7 1.532 +0.568 1.2 0.28 4.3 0.0 0.00 0.0 GRO J1655-40 253.409 -39.860 6.2 344.926 +2.502 4.0 1.02 3.9 0.0 0.00 0.0 IGR J17445-2747 266.145 -27.730 6.3 0.909 +0.825 1.1 0.00 3.8 0.0 0.00 0.0 IGR J18048-1455 271.285 -14.888 6.5 14.416 +3.177 5.5 0.00 3.7 0.0 0.00 0.0 GX 13+1 273.586 -17.075 5.8 13.568 +0.184 3.4 0.81 4.2 0.0 0.00 0.0 SGR J1745-29 266.503 -29.025 7.5 359.968 -0.120 1.1 0.33 3.2 0.0 0.00 0.0 IGR J17488-2338 267.049 -23.549 6.6 4.907 +2.299 1.2 0.00 3.7 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 1742-294 266.493 -29.526 359.536 -0.373 2.3 0.22 10.5 0.6 0.13 4.8 1E 1740.7-2942 265.972 -29.743 359.115 -0.100 1.5 0.21 7.3 1.0 0.13 7.8 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.5 0.23 6.8 0.4 0.13 3.0 4U 1722-30 261.888 -30.802 356.320 +2.298 2.0 0.34 6.0 0.8 0.23 3.2 GX 3+1 266.988 -26.555 2.303 +0.795 24.5 0.38 64.8 2.7 0.18 15.0 GX 354-0 263.000 -33.835 354.307 -0.158 12.3 0.71 17.3 4.1 0.55 7.6 GX 5-1 270.284 -25.077 5.079 -1.017 126.1 1.83 68.9 11.1 0.79 14.0 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.8 0.29 6.1 0.5 0.17 2.8 SLX 1744-299_300 266.869 -30.026 359.278 -0.911 2.3 0.22 10.2 0.5 0.13 3.5 Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 0.7 0.22 3.4 0.2 0.13 1.4 NEW SOURCE 268.026 -23.006 5.834 +1.806 13.6 2.13 6.4 2.4 1.28 1.9 NEW SOURCE 265.668 -24.020 3.847 +3.134 4.9 0.78 6.3 0.0 0.00 0.0 NEW SOURCE 269.824 -23.743 6.029 +0.009 11.9 2.19 5.4 1.6 1.11 1.4 NEW SOURCE 261.377 -25.131 0.798 +5.821 0.0 0.00 0.0 3.4 1.10 3.1