Revolution 0364: Observation start 2005-10-06T08:44 = MJD 53649.364
Total Observation GTI = 12854 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GX 5-1 270.289 -25.079 0.7 5.080 -1.022 17.1 0.33 51.4 0.0 0.00 0.0
GRS 1758-258 270.304 -25.741 0.7 4.511 -1.362 13.7 0.29 47.6 10.0 0.23 42.8
Ginga 1826-24 277.367 -23.793 0.9 9.276 -6.085 18.7 0.51 36.5 6.8 0.39 17.3
4U 1700-377 255.989 -37.847 1.2 347.753 +2.170 18.2 0.71 25.8 4.0 0.54 7.4
1E 1740.7-2942 265.989 -29.751 1.2 359.116 -0.117 7.8 0.31 25.2 5.0 0.26 19.5
OAO 1657-415 255.192 -41.649 1.3 344.370 +0.330 32.8 1.41 23.2 6.6 1.02 6.4
GX 1+4 263.007 -24.748 1.2 1.934 +4.795 8.4 0.32 26.2 0.0 0.00 0.0
H 1820-303 275.918 -30.358 1.3 2.790 -7.912 9.2 0.42 22.2 0.0 0.00 0.0
GX 349+2 256.415 -36.420 2.3 349.096 +2.763 6.2 0.55 11.4 0.0 0.00 0.0
3A 1822-371 276.463 -37.133 2.9 356.831 -11.316 5.9 0.66 8.9 0.0 0.00 0.0
4U 1722-30 261.875 -30.789 2.5 356.325 +2.315 3.6 0.34 10.6 1.2 0.27 4.3
GX 354-0 262.959 -33.848 2.4 354.277 -0.136 3.9 0.35 11.2 0.0 0.00 0.0
GX 3+1 266.993 -26.568 2.7 2.295 +0.784 3.0 0.31 9.6 0.0 0.00 0.0
GX 9+1 270.375 -20.493 3.2 9.103 +1.179 3.5 0.43 8.1 0.0 0.00 0.0
SLX 1735-269 264.558 -26.994 3.4 0.790 +2.410 2.1 0.28 7.7 1.1 0.23 5.0
IGR J17252-3616 261.372 -36.243 3.0 351.564 -0.381 3.4 0.39 8.8 0.0 0.00 0.0
SLX 1744-299_300 266.857 -30.049 2.8 359.253 -0.914 2.6 0.29 9.2 1.5 0.25 6.0
GX 17+2 274.015 -14.049 3.1 16.426 +1.263 20.1 2.41 8.3 0.0 0.00 0.0
XTE J1739-285 264.966 -28.471 4.5 359.732 +1.319 1.6 0.29 5.6 1.1 0.24 4.8
1A 1742-294 266.510 -29.559 5.2 359.516 -0.403 1.4 0.30 4.7 0.0 0.00 0.0
GX 13+1 273.646 -17.154 6.3 13.527 +0.096 3.2 0.83 3.8 0.0 0.00 0.0
Swift J1749.4-2807 267.426 -28.174 6.1 1.116 -0.373 1.3 0.33 4.0 0.0 0.00 0.0
IGR J17544-2619 268.691 -26.279 6.0 3.320 -0.375 1.2 0.00 4.1 0.0 0.00 0.0
IGR J17285-2922 262.206 -29.322 5.8 357.706 +2.889 1.4 0.33 4.2 0.0 0.00 0.0
Swift J173203.1-3445 263.147 -34.773 6.2 353.588 -0.772 1.3 0.32 3.9 0.0 0.00 0.0
1A 1743-288 266.673 -28.941 5.2 0.118 -0.203 1.2 0.26 4.8 0.0 0.00 0.0
XB 1832-330 278.827 -33.050 7.3 1.438 -11.316 1.8 0.56 3.3 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 3.9 0.23 17.0 0.7 0.14 4.8
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.7 0.23 7.5 1.0 0.14 6.8
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.8 0.23 3.4 0.2 0.14 1.3
4U 1722-30 261.888 -30.802 356.320 +2.298 2.2 0.49 4.5 0.4 0.37 1.1
GRS 1734-292 264.367 -29.142 358.883 +1.404 1.0 0.26 4.1 0.2 0.16 1.3
GX 3+1 266.982 -26.568 2.289 +0.792 21.4 0.36 58.9 2.2 0.19 11.4
GX 354-0 262.994 -33.827 354.311 -0.149 13.5 1.03 13.2 3.0 0.80 3.7
GX 5-1 270.291 -25.074 5.085 -1.022 121.7 1.60 76.2 17.2 0.74 23.2
SLX 1735-269 264.571 -26.994 0.796 +2.400 1.4 0.30 4.7 0.5 0.18 2.6
SLX 1737-282 265.163 -28.297 359.971 +1.264 0.9 0.24 3.6 0.3 0.14 2.0
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.5 0.22 6.6 0.4 0.14 3.0
XTE J1739-285 264.975 -28.496 359.714 +1.298 2.2 0.25 9.0 0.4 0.15 2.5
NEW SOURCE 271.213 -25.814 4.850 -2.110 7.5 1.35 5.5 0.8 0.66 1.2
NEW SOURCE 272.790 -26.241 5.162 -3.557 9.0 2.59 3.5 0.0 0.00 0.0
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