INTEGRAL Galactic bulge Monitoring
Revolution 0348: Observation start 1999-12-31T23:58 = MJD 51544
Total Observation GTI = 11877 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 ==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== ===== H 1820-303 275.920 -30.358 0.8 2.792 -7.913 17.7 0.44 40.0 4.0 0.34 11.8 GRS 1758-258 270.295 -25.750 0.8 4.499 -1.359 12.5 0.31 40.3 8.3 0.24 33.8 IGR J17464-3213 266.573 -32.237 0.9 357.256 -1.841 12.2 0.33 37.1 5.0 0.27 18.7 GX 5-1 270.283 -25.083 0.9 5.073 -1.019 11.2 0.30 37.2 0.0 0.00 0.0 Ginga 1826-24 277.373 -23.799 1.0 9.272 -6.093 19.4 0.59 33.0 7.9 0.44 17.9 1E 1740.7-2942 265.991 -29.736 1.1 359.130 -0.110 7.5 0.28 26.4 5.0 0.23 21.5 GX 349+2 256.439 -36.430 1.2 349.100 +2.742 12.7 0.53 23.9 0.0 0.00 0.0 4U 1700-377 255.979 -37.840 1.3 347.754 +2.181 16.4 0.74 22.1 4.3 0.56 7.7 GX 354-0 262.973 -33.840 1.5 354.290 -0.142 6.2 0.32 19.5 0.0 0.00 0.0 GRO J1655-40 253.483 -39.821 1.8 344.993 +2.482 17.0 1.08 15.7 6.9 0.79 8.7 GX 17+2 274.021 -14.047 2.0 16.430 +1.259 27.9 2.05 13.6 0.0 0.00 0.0 GX 9+1 270.389 -20.561 2.2 9.051 +1.134 5.3 0.43 12.5 0.0 0.00 0.0 4U 1722-30 261.866 -30.816 2.4 356.298 +2.306 3.6 0.31 11.4 1.9 0.26 7.5 KS 1741-293 266.239 -29.316 0.0 359.600 -0.075 3.0 0.00 11.0 1.1 0.22 4.9 MXB 1730-335 263.355 -33.381 2.3 354.849 -0.158 3.6 0.31 11.9 0.0 0.00 0.0 XTE J1818-245 274.593 -24.511 2.8 7.464 -4.172 4.4 0.46 9.5 2.1 0.35 6.0 GX 1+4 262.985 -24.762 2.8 1.911 +4.804 3.1 0.33 9.3 0.0 0.00 0.0 SLX 1744-299_300 266.884 -30.013 3.8 359.296 -0.916 2.0 0.30 6.7 1.4 0.23 5.9 GX 13+1 273.656 -17.170 3.6 13.517 +0.080 5.0 0.70 7.1 0.0 0.00 0.0 3A 1822-371 276.436 -37.128 4.2 356.826 -11.294 3.7 0.62 6.1 0.0 0.00 0.0 SLX 1735-269 264.572 -26.980 3.6 0.808 +2.407 2.2 0.31 7.2 1.5 0.25 6.1 1E 1743.1-2843 266.618 -28.720 5.0 0.281 -0.047 1.6 0.32 5.0 0.0 0.00 0.0 GX 3+1 266.971 -26.532 0.0 2.315 +0.820 1.3 0.00 4.5 0.0 0.00 0.0 GRS 1734-292 264.359 -29.043 4.7 358.964 +1.463 1.4 0.27 5.2 0.0 0.00 0.0 3A 1728-169 262.956 -16.895 5.4 8.581 +9.056 2.7 0.59 4.5 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 1742-294 266.515 -29.506 359.563 -0.379 3.5 0.27 13.1 0.6 0.15 3.8 1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.0 0.27 7.2 1.1 0.16 7.1 1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.1 0.26 4.4 0.3 0.14 2.4 GX 3+1 266.975 -26.565 2.289 +0.799 17.6 0.35 50.8 2.0 0.17 11.5 GX 354-0 262.989 -33.835 354.302 -0.150 10.9 1.88 5.8 2.1 1.13 1.9 GX 5-1 270.297 -25.077 5.084 -1.028 124.5 1.60 77.7 14.0 0.68 20.7 IGR J17464-3213 266.565 -32.234 357.255 -1.833 12.9 0.45 28.6 2.0 0.25 7.8 MXB 1730-335 263.350 -33.388 354.841 -0.158 16.5 1.34 12.3 2.4 0.75 3.2 SLX 1735-269 264.571 -26.994 0.796 +2.400 1.5 0.30 5.0 0.5 0.17 2.7 XTE J1739-285 264.975 -28.496 359.714 +1.298 2.7 0.26 10.5 0.3 0.14 1.9 NEW SOURCE 266.936 -22.614 5.656 +2.870 10.8 1.74 6.2 1.7 0.96 1.8 NEW SOURCE 268.493 -23.843 5.331 +1.012 6.8 1.16 5.9 0.0 0.00 0.0 NEW SOURCE 266.433 -23.113 4.988 +3.008 6.7 1.27 5.2 0.0 0.00 0.0 NEW SOURCE 268.834 -26.376 3.301 -0.535 0.0 0.00 0.0 0.7 0.23 3.2