Revolution 0593: Observation start 2007-08-22T02:53 = MJD 54334.121
Total Observation GTI = 12377 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 1700-377 255.974 -37.848 0.8 347.745 +2.179 28.8 0.71 40.4 8.0 0.55 14.5
GX 1+4 263.007 -24.739 0.9 1.942 +4.800 13.1 0.34 38.1 0.0 0.00 0.0
Ginga 1826-24 277.370 -23.795 1.1 9.275 -6.089 17.2 0.64 26.9 6.2 0.49 12.6
H 1820-303 275.918 -30.365 1.3 2.784 -7.915 10.5 0.48 22.1 0.0 0.00 0.0
GX 349+2 256.429 -36.441 1.6 349.087 +2.742 11.6 0.65 17.9 0.0 0.00 0.0
GRS 1758-258 270.305 -25.742 1.8 4.510 -1.363 5.6 0.36 15.7 2.6 0.30 8.8
4U 1722-30 261.913 -30.797 2.3 356.336 +2.283 4.4 0.38 11.4 0.0 0.00 0.0
GX 3+1 266.995 -26.573 2.4 2.291 +0.780 3.5 0.32 11.2 0.0 0.00 0.0
GX 5-1 270.294 -25.092 0.0 5.071 -1.032 3.4 0.00 9.5 0.0 0.00 0.0
GX 17+2 274.001 -14.039 2.6 16.427 +1.281 27.5 2.68 10.3 0.0 0.00 0.0
GX 354-0 262.992 -33.848 2.5 354.292 -0.159 3.7 0.35 10.6 0.0 0.00 0.0
GX 9+1 270.380 -20.504 2.8 9.096 +1.170 4.2 0.45 9.4 0.0 0.00 0.0
SAX J1810.8-2609 272.678 -26.178 3.1 5.170 -3.439 3.3 0.39 8.5 0.0 0.00 0.0
SLX 1735-269 264.572 -26.977 3.1 0.811 +2.409 2.9 0.35 8.2 1.5 0.29 5.0
3A 1822-371 276.439 -37.090 3.3 356.862 -11.280 5.3 0.68 7.9 0.0 0.00 0.0
IGR J17091-3624 257.345 -36.452 4.3 349.519 +2.145 3.6 0.62 5.8 0.0 0.00 0.0
Swift J174535.5-2901 266.422 -29.050 4.5 359.911 -0.072 1.7 0.30 5.6 0.0 0.00 0.0
GX 13+1 273.700 -17.106 4.3 13.593 +0.073 4.4 0.00 5.8 0.0 0.00 0.0
H 1702-429 256.511 -43.000 4.2 343.892 -1.266 12.4 2.07 6.0 7.5 1.55 4.8
SLX 1744-299_300 266.826 -30.110 5.6 359.187 -0.922 1.4 0.32 4.4 0.0 0.00 0.0
SAX J1712.6-3739 258.183 -37.684 4.6 348.920 +0.877 3.4 0.62 5.5 0.0 0.00 0.0
AX J1736.4-2910 264.250 -29.209 5.2 358.773 +1.455 1.5 0.31 4.7 0.0 0.00 0.0
IGR J17252-3616 261.281 -36.226 6.3 351.536 -0.311 1.8 0.48 3.8 0.0 0.00 0.0
PKS 1830-211 278.333 -21.133 4.8 12.066 -5.675 4.2 0.82 5.1 0.0 0.00 0.0
XTE J1720-318 259.879 -31.786 6.3 354.537 +3.162 1.5 0.39 3.9 0.0 0.00 0.0
1RXS J165443.5-19162 262.535 -19.375 5.7 6.245 +8.067 2.4 0.56 4.3 0.0 0.00 0.0
IGR J17511-3057 267.837 -30.888 6.6 358.967 -2.070 1.3 0.00 3.7 0.0 0.00 0.0
4U 1705-32 257.313 -32.292 0.0 352.856 +4.637 1.7 0.00 3.6 0.0 0.00 0.0
SAX J1750.8-2900 267.623 -28.999 6.8 0.497 -0.945 1.1 0.00 3.5 0.0 0.00 0.0
1A 1742-294 266.494 -29.498 0.0 359.561 -0.359 1.0 0.00 3.5 0.0 0.00 0.0
IGR J17451-3022 266.400 -30.403 0.0 358.746 -0.760 1.1 0.00 3.4 0.0 0.00 0.0
MXB 1730-335 263.341 -33.439 6.3 354.794 -0.179 1.3 0.34 3.9 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 -29.525 359.551 -0.394 5.2 0.32 16.4 1.0 0.19 5.2
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 1.2 0.33 3.8 0.0 0.00 0.0
GX 3+1 266.980 -26.569 2.287 +0.793 39.7 0.51 77.4 4.5 0.25 17.9
GX 354-0 262.989 -33.835 354.302 -0.150 15.7 1.36 11.5 1.9 1.03 1.9
GX 5-1 270.284 -25.080 5.076 -1.018 92.0 1.79 51.4 5.3 0.74 7.2
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.2 0.32 6.9 0.6 0.19 3.0
NEW SOURCE 267.894 -22.932 5.835 +1.948 14.1 2.92 4.8 0.0 0.00 0.0
NEW SOURCE 266.546 -24.016 4.269 +2.451 4.5 1.05 4.3 0.0 0.00 0.0
NEW SOURCE 272.775 -26.080 5.298 -3.468 15.7 3.30 4.8 0.0 0.00 0.0
NEW SOURCE 265.555 -23.917 3.880 +3.275 5.1 1.13 4.5 0.0 0.00 0.0
NEW SOURCE 271.792 -26.025 4.920 -2.668 8.7 2.21 4.0 0.0 0.00 0.0
NEW SOURCE 271.012 -26.648 4.034 -2.362 3.8 0.93 4.1 0.0 0.00 0.0
NEW SOURCE 267.981 -26.054 3.190 +0.288 2.5 0.60 4.2 0.0 0.00 0.0
NEW SOURCE 269.460 -23.986 5.652 +0.175 7.6 1.89 4.0 0.0 0.00 0.0
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