Revolution 1224: Observation start 2012-10-23T04:37 = MJD 56223.193
Total Observation GTI = 15754 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 266.296 -26.406 0.3 2.110 +1.401 51.2 0.30 172.6 21.6 0.21 100.6
4U 1700-377 255.981 -37.846 0.5 347.750 +2.176 50.6 0.61 83.3 15.4 0.41 37.8
IGR J17464-3213 266.577 -32.243 0.9 357.252 -1.847 11.0 0.30 36.6 7.6 0.22 35.4
GX 1+4 263.009 -24.753 1.2 1.931 +4.791 9.2 0.36 25.8 0.0 0.00 0.0
GX 5-1 270.295 -25.084 1.3 5.078 -1.029 8.6 0.39 22.0 0.0 0.00 0.0
Ginga 1826-24 277.401 -23.780 1.6 9.302 -6.108 12.7 0.72 17.7 6.7 0.48 14.0
GX 349+2 256.455 -36.426 1.6 349.110 +2.734 9.1 0.50 18.3 0.0 0.00 0.0
IGR J17091-3624 257.302 -36.414 2.2 349.529 +2.195 5.8 0.48 12.1 4.4 0.33 13.6
GRS 1758-258 270.303 -25.763 2.3 4.491 -1.372 4.2 0.36 11.8 4.2 0.25 16.7
GX 354-0 263.024 -33.810 2.4 354.339 -0.161 4.1 0.36 11.3 0.0 0.00 0.0
1E 1740.7-2942 265.994 -29.785 2.6 359.089 -0.138 3.4 0.33 10.0 1.5 0.24 6.2
3A 1822-371 276.379 -37.082 2.9 356.848 -11.233 6.8 0.75 9.0 0.0 0.00 0.0
SAX J1806.5-2215 271.669 -22.229 3.3 8.184 -0.723 3.4 0.44 7.8 1.9 0.30 6.4
4U 1722-30 261.921 -30.838 3.3 356.306 +2.255 2.4 0.00 7.8 1.3 0.22 5.8
H 1820-303 275.906 -30.333 4.7 2.808 -7.891 2.8 0.53 5.2 0.0 0.00 0.0
IGR J18027-2016 270.622 -20.351 4.3 9.341 +1.048 3.0 0.51 5.8 0.0 0.00 0.0
GX 3+1 267.007 -26.583 0.0 2.288 +0.766 1.7 0.00 5.7 0.0 0.00 0.0
GRS 1747-312 267.643 -31.243 4.6 358.577 -2.108 1.6 0.30 5.4 0.0 0.00 0.0
IGR J17456-2901 266.396 -28.974 0.0 359.963 -0.013 1.8 0.00 5.3 0.0 0.00 0.0
XTE J1739-285 264.937 -28.579 5.4 359.627 +1.282 1.4 0.30 4.6 0.0 0.00 0.0
IGR J17536-2339 268.376 -23.692 4.8 5.407 +1.181 1.8 0.36 5.1 0.0 0.00 0.0
NEW SOURCE 261.979 -33.085 3.9 354.463 +0.966 2.0 0.32 6.4 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 6.1 0.23 26.0 1.1 0.13 8.3
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.3 0.22 5.8 0.4 0.13 3.0
4U 1722-30 261.888 -30.802 356.320 +2.298 2.5 0.25 10.0 0.6 0.16 3.8
GRS 1734-292 264.367 -29.142 358.883 +1.404 0.7 0.19 3.6 0.3 0.11 2.6
GRS 1747-312 267.690 -31.292 358.555 -2.168 4.2 0.32 13.0 0.7 0.19 3.6
GRS 1758-258 270.303 -25.741 4.511 -1.361 7.1 1.75 4.1 1.9 0.89 2.1
GX 1+4 263.009 -24.746 1.937 +4.795 4.5 0.44 10.3 1.9 0.28 6.7
GX 3+1 266.986 -26.566 2.293 +0.791 44.6 0.46 97.1 4.1 0.23 17.3
GX 354-0 262.989 -33.835 354.302 -0.150 9.0 0.59 15.3 1.7 0.42 4.1
GX 5-1 270.278 -25.086 5.068 -1.017 138.6 2.64 52.4 18.7 1.39 13.4
IGR J17464-3213 266.567 -32.229 357.260 -1.832 1.8 0.34 5.2 1.5 0.21 7.3
SLX 1735-269 264.571 -26.994 0.796 +2.400 0.8 0.25 3.1 0.3 0.14 2.4
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.25 4.3 0.3 0.14 2.2
Swift J174510.8-2624 266.296 -26.405 2.110 +1.401 54.6 0.44 125.5 12.4 0.24 52.5
XTE J1739-285 264.975 -28.496 359.714 +1.298 0.6 0.20 3.0 0.2 0.11 1.4
NEW SOURCE 266.176 -23.696 4.367 +2.907 14.4 2.54 5.7 2.1 1.51 1.4
NEW SOURCE 264.663 -26.985 0.848 +2.336 1.8 0.25 7.2 0.0 0.00 0.0
NEW SOURCE 263.314 -26.247 0.822 +3.750 1.4 0.28 5.1 0.2 0.17 1.4
NEW SOURCE 267.431 -25.883 3.084 +0.800 3.2 0.58 5.5 0.7 0.32 2.2
NEW SOURCE 263.800 -29.106 358.648 +1.841 0.7 0.20 3.5 0.3 0.12 2.8
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