Revolution 0544: Observation start 1999-12-31T23:58 = MJD 51544
Total Observation GTI = 9788 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 1700-377 255.993 -37.845 0.6 347.757 +2.169 52.7 0.94 56.1 14.1 0.70 20.0
GX 1+4 263.000 -24.746 0.8 1.933 +4.802 19.9 0.49 41.1 0.0 0.00 0.0
GRS 1758-258 270.304 -25.753 1.1 4.500 -1.367 11.6 0.42 27.3 8.7 0.34 25.4
Ginga 1826-24 277.355 -23.806 1.1 9.259 -6.081 16.7 0.63 26.5 7.0 0.49 14.3
1E 1740.7-2942 265.987 -29.744 1.2 359.121 -0.112 10.3 0.41 25.0 6.3 0.34 18.6
GX 5-1 270.281 -25.092 1.3 5.065 -1.022 10.3 0.45 22.8 0.0 0.00 0.0
H 1820-303 275.911 -30.362 1.5 2.784 -7.908 10.1 0.52 19.4 0.0 0.00 0.0
GX 349+2 256.474 -36.422 1.7 349.123 +2.725 12.4 0.76 16.4 0.0 0.00 0.0
1A 1742-294 266.473 -29.516 2.0 359.536 -0.353 5.2 0.38 13.8 1.4 0.00 4.7
GX 354-0 262.986 -33.828 1.9 354.307 -0.144 6.7 0.46 14.4 0.0 0.00 0.0
3A 1822-371 276.451 -37.109 2.5 356.849 -11.297 7.4 0.68 10.9 2.6 0.52 5.1
4U 1722-30 261.892 -30.795 2.6 356.328 +2.299 4.3 0.43 10.1 0.0 0.00 0.0
GX 3+1 266.980 -26.562 3.1 2.294 +0.797 3.0 0.36 8.5 0.0 0.00 0.0
GX 17+2 273.981 -14.046 3.2 16.412 +1.294 23.2 2.85 8.1 0.0 0.00 0.0
GX 9+1 270.368 -20.564 3.2 9.039 +1.150 4.3 0.52 8.2 0.0 0.00 0.0
OAO 1657-415 255.185 -41.658 2.8 344.359 +0.329 22.2 2.36 9.4 0.0 0.00 0.0
IGR J17456-2901 266.449 -28.970 3.3 359.991 -0.050 2.9 0.37 7.8 0.0 0.00 0.0
SLX 1735-269 264.628 -27.049 4.4 0.776 +2.328 2.0 0.36 5.6 0.0 0.00 0.0
SLX 1737-282 265.082 -28.292 5.1 359.938 +1.326 1.9 0.39 4.9 0.0 0.00 0.0
4U 1735-444 264.725 -44.435 4.5 346.061 -6.975 18.5 3.35 5.5 0.0 0.00 0.0
GX 13+1 273.570 -17.121 5.4 13.520 +0.175 4.2 0.00 4.5 0.0 0.00 0.0
SLX 1744-299_300 266.876 -29.999 5.1 359.305 -0.903 1.9 0.38 4.8 0.0 0.00 0.0
IGR J17177-3656 259.325 -37.013 5.6 349.996 +0.531 2.7 0.61 4.4 0.0 0.00 0.0
HETE J1900.1-2455 284.948 -24.833 0.0 11.354 -12.764 10.4 0.00 4.1 0.0 0.00 0.0
3A 1728-169 262.935 -17.019 5.5 8.464 +9.006 4.7 1.05 4.5 0.0 0.00 0.0
XB 1832-330 278.844 -32.983 7.3 1.506 -11.301 2.2 0.66 3.3 0.0 0.00 0.0
IGR J17497-2821 267.313 -28.396 7.6 0.874 -0.402 1.2 0.37 3.2 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 0.37 3.6 0.8 0.23 3.4
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.39 5.4 1.1 0.24 4.4
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.4 0.39 3.7 0.6 0.23 2.5
GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 1.7 0.39 4.2 0.3 0.23 1.5
GX 3+1 266.985 -26.559 2.299 +0.794 39.2 0.65 60.5 4.1 0.30 13.6
GX 354-0 262.989 -33.835 354.302 -0.150 18.8 3.54 5.3 3.1 2.40 1.3
GX 5-1 270.286 -25.081 5.077 -1.021 115.4 1.61 71.9 10.5 0.64 16.4
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.6 0.36 4.4 0.4 0.22 1.6
NEW SOURCE 271.042 -28.173 2.716 -3.131 2.8 0.56 5.0 0.4 0.30 1.5
NEW SOURCE 271.096 -25.707 4.892 -1.966 5.6 1.14 4.9 0.0 0.00 0.0
NEW SOURCE 272.803 -24.519 6.682 -2.742 20.0 4.61 4.3 5.3 2.39 2.2
NEW SOURCE 271.976 -27.263 3.914 -3.411 4.6 0.93 5.0 0.9 0.50 1.9
NEW SOURCE 271.451 -31.587 359.896 -5.099 2.8 0.60 4.6 0.0 0.00 0.0
NEW SOURCE 268.598 -22.978 6.126 +1.366 11.5 3.11 3.7 4.9 1.70 2.9
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