Revolution 1261: Observation start 2013-02-11T00:55 = MJD 56334.039
Total Observation GTI = 12400 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
Swift J174510.8-2624 266.297 -26.400 0.9 2.115 +1.404 13.2 0.35 38.0 9.9 0.26 38.0
GX 5-1 270.286 -25.089 1.1 5.069 -1.025 10.9 0.37 29.0 0.0 0.00 0.0
GRS 1758-258 270.289 -25.751 1.1 4.495 -1.355 10.1 0.35 28.3 5.7 0.26 22.0
Swift J1753.7-2544 268.413 -25.750 1.2 3.649 +0.108 9.1 0.35 25.7 6.2 0.25 24.4
Ginga 1826-24 277.388 -23.801 1.3 9.278 -6.107 14.6 0.66 22.0 5.8 0.45 12.8
XTE J1810-189 272.591 -19.068 1.4 11.366 +0.056 12.3 0.60 20.3 3.1 0.42 7.3
GX 3+1 266.974 -26.559 2.3 2.294 +0.803 3.8 0.33 11.8 0.0 0.00 0.0
OAO 1657-415 255.201 -41.662 2.6 344.364 +0.317 15.4 1.50 10.3 0.0 0.00 0.0
GX 349+2 256.483 -36.411 2.6 349.137 +2.725 6.2 0.62 10.0 0.0 0.00 0.0
SLX 1735-269 264.551 -27.019 3.0 0.766 +2.402 2.8 0.32 8.7 1.5 0.24 6.2
H 1820-303 275.915 -30.345 3.0 2.801 -7.904 4.1 0.48 8.7 0.0 0.00 0.0
GX 17+2 274.005 -14.040 3.1 16.428 +1.276 23.1 2.76 8.4 0.0 0.00 0.0
GX 13+1 273.633 -17.140 3.5 13.533 +0.114 7.2 0.99 7.3 0.0 0.00 0.0
SLX 1744-299_300 266.866 -29.975 3.9 359.320 -0.883 2.3 0.35 6.4 0.0 0.00 0.0
GX 9+1 270.329 -20.536 3.4 9.045 +1.195 3.4 0.46 7.4 0.0 0.00 0.0
4U 1722-30 261.891 -30.796 3.0 356.326 +2.300 3.2 0.37 8.5 0.0 0.00 0.0
3A 1822-371 276.426 -37.125 3.4 356.826 -11.285 4.9 0.64 7.6 0.0 0.00 0.0
GX 1+4 263.017 -24.737 3.9 1.948 +4.794 2.6 0.40 6.4 0.0 0.00 0.0
SAX J1806.5-2215 271.615 -22.236 3.7 8.153 -0.683 3.1 0.46 6.8 0.0 0.00 0.0
KS 1741-293 266.212 -29.333 0.0 359.574 -0.063 1.9 0.00 5.8 0.0 0.00 0.0
GX 354-0 263.000 -33.820 4.4 354.320 -0.150 2.2 0.39 5.6 0.0 0.00 0.0
SLX 1746-331 267.381 -33.107 5.7 356.861 -2.872 1.5 0.00 4.3 0.0 0.00 0.0
GRS 1734-292 264.263 -29.184 5.2 358.800 +1.458 1.5 0.31 4.8 1.0 0.24 4.3
XTE J1752-223 268.167 -22.277 0.0 6.529 +2.065 1.8 0.00 4.0 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 7.7 0.26 29.3 1.3 0.13 9.5
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.6 0.26 6.1 0.3 0.13 2.4
GX 3+1 266.984 -26.566 2.292 +0.792 62.2 0.42 147.3 7.7 0.19 41.0
GX 354-0 262.989 -33.835 354.302 -0.150 9.0 0.97 9.2 2.6 0.74 3.5
GX 5-1 270.289 -25.081 5.077 -1.023 129.9 1.52 85.4 16.5 0.65 25.2
SLX 1735-269 264.571 -26.994 0.796 +2.400 1.3 0.35 3.6 0.4 0.17 2.5
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.9 0.26 7.5 0.4 0.14 2.8
XTE J1739-285 264.972 -28.482 359.725 +1.308 11.7 0.27 42.6 1.5 0.14 11.2
Swift J174510.8-2624 266.289 -26.402 2.110 +1.409 3.5 0.38 9.3 1.8 0.18 9.8
NEW SOURCE 270.903 -25.268 5.189 -1.599 8.6 1.46 5.9 1.0 0.65 1.5
NEW SOURCE 269.334 -24.504 5.146 +0.016 6.1 1.25 4.9 0.9 0.57 1.5
NEW SOURCE 268.411 -28.099 1.624 -1.081 1.4 0.32 4.5 0.2 0.16 1.3
Swift J1753.7-2544 268.422 -25.756 3.648 +0.097 1.7 0.57 3.1 1.3 0.27 4.8
NEW SOURCE 268.058 -27.714 1.798 -0.617 1.0 0.33 3.0 0.5 0.16 2.9
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