Revolution 1093: Observation start 2011-09-26T16:19 = MJD 55830.681
Total Observation GTI = 11648 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 1700-377 255.985 -37.846 0.7 347.752 +2.174 57.8 1.05 55.1 16.1 0.74 21.6
GX 5-1 270.270 -25.075 1.1 5.074 -1.006 11.7 0.42 27.6 1.2 0.00 3.6
GX 354-0 262.997 -33.843 1.2 354.299 -0.161 11.3 0.45 25.4 2.9 0.33 8.7
1E 1740.7-2942 265.989 -29.734 1.3 359.130 -0.107 8.5 0.37 23.4 5.8 0.29 20.2
GRS 1758-258 270.299 -25.745 1.8 4.505 -1.360 6.1 0.39 15.8 5.0 0.29 17.1
Ginga 1826-24 277.389 -23.789 1.8 9.289 -6.102 11.1 0.72 15.5 4.5 0.51 8.8
GX 349+2 256.435 -36.435 2.3 349.093 +2.741 8.2 0.70 11.7 0.0 0.00 0.0
3A 1822-371 276.420 -37.050 2.3 356.892 -11.249 9.5 0.83 11.4 0.0 0.00 0.0
MAXI J1836-194 278.943 -19.286 2.6 13.980 -5.349 13.7 1.33 10.3 8.2 0.92 8.9
H 1820-303 275.962 -30.359 2.9 2.807 -7.946 5.2 0.59 8.8 0.0 0.00 0.0
GX 1+4 263.010 -24.733 2.9 1.948 +4.801 3.6 0.40 9.0 0.0 0.00 0.0
GX 3+1 266.948 -26.612 3.4 2.236 +0.796 3.1 0.41 7.6 0.0 0.00 0.0
4U 1722-30 261.901 -30.779 3.1 356.345 +2.302 3.5 0.42 8.3 1.4 0.32 4.3
GX 9+1 270.374 -20.489 3.8 9.106 +1.183 3.4 0.50 6.8 0.0 0.00 0.0
XB 1733-30 263.920 -30.457 5.1 357.566 +1.024 1.8 0.37 4.9 0.0 0.00 0.0
GRS 1747-312 267.677 -31.271 6.2 358.568 -2.147 1.6 0.42 3.9 0.0 0.00 0.0
MXB 1730-335 263.399 -33.415 0.0 354.841 -0.207 2.1 0.00 4.7 0.0 0.00 0.0
GX 17+2 274.024 -14.078 0.0 16.404 +1.242 9.9 0.00 4.7 0.0 0.00 0.0
Swift J173203.1-3445 262.972 -34.707 0.0 353.565 -0.615 2.2 0.00 4.5 0.0 0.00 0.0
XTE J1751-305 267.784 -30.653 5.2 359.147 -1.911 1.7 0.36 4.8 0.0 0.00 0.0
IGR J17252-3616 261.300 -36.240 4.9 351.534 -0.332 2.8 0.55 5.1 0.0 0.00 0.0
SLX 1744-299_300 266.882 -29.934 5.3 359.363 -0.874 1.7 0.36 4.7 0.0 0.00 0.0
SLX 1735-269 264.574 -27.034 4.4 0.764 +2.377 2.4 0.42 5.7 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined 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+2 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 5.3 0.31 17.3 0.9 0.18 4.8
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 2.1 0.30 7.1 1.1 0.18 6.2
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.6 0.29 5.3 0.3 0.17 2.0
GX 3+1 266.988 -26.559 2.299 +0.793 50.0 0.39 128.0 4.8 0.20 23.6
GX 354-0 262.989 -33.835 354.302 -0.150 12.6 2.21 5.7 3.2 1.75 1.8
GX 5-1 270.279 -25.072 5.081 -1.011 122.8 1.57 78.3 17.2 0.79 21.7
SLX 1735-269 264.571 -26.994 0.796 +2.400 1.1 0.29 3.9 0.3 0.17 1.8
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 3.3 0.33 10.0 0.7 0.20 3.4
CONFUSED ID 266.986 -26.563 2.295 +0.792 50.2 0.39 128.4 4.9 0.20 24.1
NEW SOURCE 272.541 -27.368 4.064 -3.902 9.0 2.05 4.4 0.0 0.00 0.0
CONFUSED ID 266.990 -26.490 2.360 +0.827 16.9 0.37 46.2 1.4 0.20 7.1
NEW SOURCE 272.394 -27.691 3.717 -3.942 7.8 1.88 4.1 0.0 0.00 0.0
CONFUSED ID 266.907 -26.566 2.256 +0.851 17.3 0.36 48.4 1.7 0.20 8.8
NEW SOURCE 265.604 -24.139 3.715 +3.121 2.3 0.56 4.1 0.0 0.00 0.0
NEW SOURCE 270.504 -25.126 5.135 -1.215 5.8 1.42 4.1 0.0 0.00 0.0
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