Revolution 1341: Observation start 2013-10-08T07:00 = MJD 56573.292
Total Observation GTI = 12118 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 1+4 263.016 -24.750 0.6 1.937 +4.787 22.2 0.35 62.6 0.0 0.00 0.0
Ginga 1826-24 277.371 -23.797 1.0 9.274 -6.090 17.8 0.55 32.4 7.3 0.37 20.0
GRS 1758-258 270.301 -25.740 1.0 4.511 -1.359 10.8 0.34 31.8 7.7 0.24 32.2
GX 5-1 270.273 -25.088 1.4 5.064 -1.014 7.3 0.37 20.0 0.0 0.00 0.0
GX 349+2 256.421 -36.445 2.0 349.080 +2.744 9.8 0.71 13.8 0.0 0.00 0.0
H 1820-303 275.889 -30.372 1.9 2.767 -7.895 6.6 0.45 14.6 0.0 0.00 0.0
GX 354-0 262.965 -33.851 2.8 354.278 -0.142 3.8 0.41 9.3 0.0 0.00 0.0
SLX 1735-269 264.584 -27.039 2.7 0.764 +2.366 3.4 0.35 9.7 1.2 0.24 4.7
SAX J1806.5-2215 271.638 -22.194 3.4 8.200 -0.681 3.2 0.42 7.7 0.0 0.00 0.0
3A 1822-371 276.443 -37.133 3.7 356.824 -11.301 4.7 0.69 6.8 2.2 0.45 5.0
OAO 1657-415 255.190 -41.666 3.1 344.355 +0.321 27.2 3.26 8.3 0.0 0.00 0.0
1E 1740.7-2942 265.971 -29.754 3.1 359.105 -0.105 2.7 0.33 8.4 1.4 0.24 5.8
GX 17+2 274.010 -14.078 3.7 16.397 +1.254 11.0 1.62 6.8 0.0 0.00 0.0
SLX 1744-299_300 266.848 -30.030 4.3 359.266 -0.898 1.9 0.33 5.8 1.2 0.24 5.1
1A 1742-294 266.491 -29.494 5.1 359.562 -0.354 1.6 0.33 4.9 0.0 0.00 0.0
1E 1742.8-2853 266.490 -28.968 4.6 0.011 -0.080 1.9 0.36 5.5 0.0 0.00 0.0
XTE J1710-281 257.581 -28.225 4.7 356.297 +6.846 2.7 0.50 5.3 0.0 0.00 0.0
V745 Sco 268.834 -33.192 6.7 357.405 -3.964 1.3 0.35 3.6 0.0 0.00 0.0
GX 9+1 270.441 -20.440 6.4 9.180 +1.152 1.7 0.44 3.8 0.0 0.00 0.0
XTE J1810-189 272.557 -19.186 6.0 11.247 +0.028 2.1 0.00 4.1 0.0 0.00 0.0
SLX 1737-282 265.104 -28.349 5.3 359.899 +1.280 1.4 0.31 4.6 1.0 0.22 4.3
IGR J17091-3624 257.282 -36.490 0.0 349.459 +2.163 2.6 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 8.3 0.27 30.8 1.4 0.14 10.0
4U 1722-30 261.888 -30.802 356.320 +2.298 3.9 0.89 4.4 1.0 0.56 1.7
GRS 1734-292 264.367 -29.142 358.883 +1.404 1.8 0.31 5.6 0.0 0.00 0.0
GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 0.8 0.27 3.2 0.0 0.00 0.0
GRS 1758-258 270.303 -25.741 4.511 -1.361 0.0 0.00 0.0 1.3 0.26 5.1
GX 1+4 263.009 -24.746 1.937 +4.795 3.6 0.82 4.4 3.1 0.48 6.4
GX 3+1 266.983 -26.559 2.298 +0.796 42.1 0.34 122.6 4.3 0.15 28.2
GX 5-1 270.293 -25.077 5.083 -1.024 127.0 0.87 145.3 12.7 0.37 34.6
SLX 1735-269 264.571 -26.994 0.796 +2.400 2.7 0.32 8.5 0.6 0.16 3.8
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.6 0.28 5.9 0.4 0.15 3.0
NEW SOURCE 268.938 -33.294 357.360 -4.090 6.1 0.88 6.9 0.0 0.00 0.0
NEW SOURCE 271.320 -24.271 6.244 -1.441 7.8 1.43 5.4 1.1 0.64 1.7
NEW SOURCE 273.133 -24.207 7.100 -2.856 19.5 3.30 5.9 0.0 0.00 0.0
NEW SOURCE 272.270 -25.253 5.805 -2.671 7.1 1.31 5.4 0.0 0.00 0.0
NEW SOURCE 266.707 -23.657 4.653 +2.511 3.3 0.71 4.6 0.6 0.34 1.6
NEW SOURCE 266.608 -21.748 6.242 +3.577 11.1 2.47 4.5 2.3 1.34 1.7
NEW SOURCE 265.886 -21.948 5.722 +4.046 8.4 2.55 3.3 3.6 1.42 2.5
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