Revolution 0370: Observation start 2005-10-26T15:33 = MJD 53669.648
Total Observation GTI = 13160 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 SOURCE
s < 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1758-258 270.297 -25.746 0.7 4.503 -1.358 15.4 0.29 52.5 9.9 0.23 42.5
GX 5-1 270.282 -25.074 0.7 5.081 -1.014 17.1 0.33 51.9 0.9 0.00 3.6
Ginga 1826-24 277.355 -23.797 1.0 9.267 -6.078 17.2 0.56 30.7 6.6 0.41 15.9
GX 1+4 263.007 -24.738 1.0 1.943 +4.801 9.5 0.32 30.1 0.0 0.00 0.0
1E 1740.7-2942 265.976 -29.740 1.1 359.119 -0.101 7.4 0.26 28.6 4.1 0.21 18.9
H 1820-303 275.917 -30.364 1.2 2.784 -7.913 10.6 0.44 24.0 0.0 0.00 0.0
IGR J17252-3616 261.306 -36.293 1.6 351.493 -0.365 6.4 0.37 17.3 0.0 0.00 0.0
GX 349+2 256.420 -36.427 2.2 349.093 +2.756 5.9 0.49 12.2 0.0 0.00 0.0
GX 354-0 262.979 -33.832 2.4 354.300 -0.141 3.4 0.30 11.3 0.0 0.00 0.0
GX 17+2 273.993 -14.039 2.8 16.424 +1.287 31.9 3.47 9.2 0.0 0.00 0.0
1A 1743-288 266.692 -28.895 2.9 0.166 -0.193 2.3 0.26 8.9 0.0 0.00 0.0
4U 1722-30 261.887 -30.780 2.9 356.338 +2.311 3.0 0.32 9.1 1.0 0.27 3.8
3A 1822-371 276.473 -37.158 3.2 356.811 -11.334 4.4 0.55 8.0 0.0 0.00 0.0
GX 9+1 270.366 -20.467 3.2 9.122 +1.200 3.1 0.38 8.0 0.0 0.00 0.0
XTE J1739-285 265.012 -28.478 4.5 359.747 +1.280 1.7 0.30 5.5 1.2 0.25 4.7
SLX 1735-269 264.622 -27.024 3.7 0.795 +2.346 1.9 0.27 6.9 0.7 0.00 3.5
GX 3+1 267.026 -26.558 4.5 2.318 +0.764 1.6 0.28 5.6 0.0 0.00 0.0
Oph Cluster 258.150 -23.296 0.0 0.653 +9.286 2.2 0.00 5.2 0.0 0.00 0.0
IGR J18135-1751 273.247 -17.836 4.9 12.745 +0.104 3.1 0.00 5.0 0.0 0.00 0.0
XB 1832-330 278.915 -33.005 5.1 1.512 -11.364 2.8 0.58 4.8 0.0 0.00 0.0
4U 1735-444 264.625 -44.407 6.3 346.047 -6.900 13.1 0.00 3.8 0.0 0.00 0.0
SLX 1744-299_300 266.845 -30.049 6.0 359.248 -0.905 1.2 0.30 4.1 0.0 0.00 0.0
GRS 1734-292 264.397 -29.177 6.1 358.868 +1.363 1.2 0.29 4.0 0.0 0.00 0.0
IGR J18027-2016 270.729 -20.219 0.0 9.505 +1.026 1.6 0.00 3.5 0.0 0.00 0.0
2E 1701.9-3723 256.417 -37.403 7.1 348.313 +2.169 1.8 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 SOURCE
s < 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 5.4 0.23 23.3 1.2 0.14 8.3
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.6 0.23 6.8 1.0 0.15 7.1
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.0 0.23 4.4 0.3 0.14 2.4
4U 1722-30 261.888 -30.802 356.320 +2.298 3.4 0.49 6.9 0.6 0.35 1.8
GX 1+4 263.009 -24.746 1.937 +4.795 2.3 0.71 3.3 1.4 0.49 2.8
GX 3+1 266.981 -26.567 2.289 +0.794 25.7 0.36 71.0 2.7 0.19 14.2
GX 354-0 262.995 -33.824 354.313 -0.148 14.1 1.01 13.9 3.0 0.83 3.6
GX 5-1 270.277 -25.072 5.081 -1.009 119.9 1.56 76.8 18.9 0.76 25.0
SLX 1735-269 264.571 -26.994 0.796 +2.400 0.9 0.28 3.2 0.0 0.00 0.0
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.3 0.23 10.0 0.4 0.15 2.5
NEW SOURCE 271.739 -26.035 4.888 -2.631 9.0 1.62 5.6 0.0 0.00 0.0
NEW SOURCE 273.134 -26.288 5.269 -3.850 15.9 3.01 5.3 2.7 1.77 1.5
NEW SOURCE 269.677 -25.745 4.227 -0.873 3.8 0.74 5.1 0.6 0.40 1.5
NEW SOURCE 266.480 -23.348 4.810 +2.850 5.2 1.13 4.6 0.0 0.00 0.0
NEW SOURCE 269.239 -26.574 3.312 -0.948 2.0 0.45 4.5 0.4 0.25 1.6
NEW SOURCE 270.522 -25.149 5.123 -1.241 5.8 1.36 4.3 0.0 0.00 0.0
NEW SOURCE 268.453 -23.195 5.871 +1.372 7.7 2.32 3.3 3.4 1.31 2.6
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