Revolution 0407: Observation start 2006-02-11T21:42 = MJD 53777.905
Total Observation GTI = 11791 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
4U 1700-377 255.979 -37.846 0.6 347.749 +2.178 44.5 0.64 69.5 11.2 0.49 23.0
GX 5-1 270.285 -25.072 0.7 5.083 -1.016 17.8 0.35 51.4 1.1 0.27 3.9
GX 1+4 263.013 -24.750 0.9 1.936 +4.790 11.7 0.33 35.2 0.0 0.00 0.0
GRS 1758-258 270.299 -25.737 1.0 4.512 -1.356 11.8 0.38 31.1 6.9 0.30 22.8
Ginga 1826-24 277.366 -23.804 1.0 9.266 -6.090 18.4 0.58 31.7 7.5 0.45 16.7
XTE J1817-330 274.419 -33.010 1.3 359.820 -7.983 9.8 0.43 22.6 3.5 0.34 10.4
1A 1742-294 266.524 -29.520 1.6 359.556 -0.392 5.3 0.31 17.3 1.5 0.25 5.8
GX 349+2 256.449 -36.414 1.7 349.118 +2.745 9.8 0.58 16.9 0.0 0.00 0.0
H 1820-303 275.928 -30.391 1.9 2.765 -7.934 6.9 0.47 14.7 0.0 0.00 0.0
4U 1722-30 261.869 -30.766 2.5 356.340 +2.332 3.4 0.31 10.8 1.5 0.25 6.1
GX 354-0 262.989 -33.837 2.0 354.300 -0.152 5.0 0.37 13.6 0.0 0.00 0.0
3A 1822-371 276.469 -37.090 2.7 356.872 -11.301 6.0 0.61 9.8 2.0 0.47 4.1
SLX 1735-269 264.601 -26.986 2.9 0.817 +2.382 2.7 0.30 9.1 1.3 0.25 5.1
GX 3+1 267.016 -26.554 2.8 2.317 +0.773 3.0 0.32 9.2 0.0 0.00 0.0
OAO 1657-415 255.211 -41.672 2.8 344.360 +0.305 14.6 1.57 9.3 0.0 0.00 0.0
GX 17+2 273.969 -14.028 3.1 16.423 +1.313 21.2 2.53 8.4 0.0 0.00 0.0
GX 13+1 273.631 -17.116 3.5 13.553 +0.127 6.4 0.87 7.4 0.0 0.00 0.0
GX 9+1 270.349 -20.595 3.8 9.003 +1.150 3.0 0.45 6.6 0.0 0.00 0.0
SGR J1745-29 266.495 -29.004 0.0 359.984 -0.103 2.1 0.00 7.4 0.0 0.00 0.0
SLX 1744-299_300 266.869 -30.022 4.9 359.282 -0.909 1.7 0.35 5.0 0.0 0.00 0.0
XTE J1739-285 265.087 -28.432 4.4 359.821 +1.249 1.8 0.32 5.7 0.0 0.00 0.0
XB 1832-330 278.978 -33.016 4.0 1.524 -11.417 4.0 0.63 6.3 0.0 0.00 0.0
GRS 1747-312 267.694 -31.302 4.4 358.549 -2.176 1.8 0.31 5.7 0.0 0.00 0.0
3A 1728-169 262.867 -17.049 0.0 8.404 +9.046 3.3 0.00 4.5 0.0 0.00 0.0
4U 1735-444 264.698 -44.448 4.7 346.039 -6.966 18.1 3.39 5.3 0.0 0.00 0.0
IGR J18135-1751 273.408 -17.876 5.8 12.783 -0.051 2.9 0.70 4.2 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 1.4 0.29 4.8 0.8 0.17 4.5
4U 1722-30 261.888 -30.802 356.320 +2.298 1.7 0.53 3.3 0.5 0.36 1.3
CONFUSED ID 267.710 -31.247 358.603 -2.160 2.8 0.36 7.8 0.5 0.22 2.4
GRS 1747-312 267.690 -31.292 358.555 -2.168 2.9 0.36 7.9 0.4 0.21 1.7
GX 1+4 263.009 -24.746 1.937 +4.795 3.5 0.91 3.8 1.6 0.58 2.8
GX 3+1 266.986 -26.559 2.299 +0.794 26.0 0.46 56.7 3.2 0.23 13.6
GX 354-0 262.989 -33.835 354.302 -0.150 21.8 1.22 17.9 3.5 0.84 4.2
GX 5-1 270.288 -25.088 5.071 -1.026 113.5 1.99 57.1 18.6 0.94 19.8
SLX 1735-269 264.571 -26.994 0.796 +2.400 1.7 0.39 4.4 0.5 0.22 2.2
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.30 3.5 0.6 0.18 3.3
Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.2 0.29 4.0 0.0 0.00 0.0
XTE J1739-285 264.975 -28.489 359.720 +1.301 7.2 0.30 23.9 0.9 0.17 5.2
NEW SOURCE 265.382 -22.535 4.975 +4.136 13.7 2.78 4.9 3.4 1.82 1.8
NEW SOURCE 268.029 -23.432 5.469 +1.587 9.1 1.76 5.2 0.0 0.00 0.0
NEW SOURCE 265.783 -22.889 4.868 +3.635 10.0 2.05 4.9 0.0 0.00 0.0
NEW SOURCE 268.167 -23.316 5.633 +1.537 8.9 1.84 4.8 1.7 1.08 1.5
NEW SOURCE 266.090 -23.027 4.898 +3.322 9.0 1.95 4.6 1.2 1.22 1.0
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