Revolution 0596: Observation start 2007-08-31T02:20 = MJD 54343.098
Total Observation GTI = 24722 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 5-1 270.278 -25.076 0.7 5.078 -1.012 12.1 0.25 49.1 1.0 0.20 5.0
GX 1+4 263.009 -24.739 0.7 1.943 +4.799 14.0 0.28 49.8 0.0 0.00 0.0
Ginga 1826-24 277.366 -23.791 0.8 9.277 -6.084 19.5 0.45 43.2 7.1 0.35 20.2
H 1820-303 275.918 -30.361 0.9 2.788 -7.913 11.2 0.33 33.9 0.0 0.00 0.0
GX 349+2 256.440 -36.425 1.2 349.104 +2.745 10.8 0.44 24.3 0.0 0.00 0.0
GX 3+1 266.973 -26.553 1.5 2.298 +0.807 4.1 0.22 18.9 0.0 0.00 0.0
GRS 1758-258 270.315 -25.745 1.9 4.512 -1.372 3.5 0.24 14.7 1.6 0.20 8.3
3A 1822-371 276.483 -37.108 1.7 356.861 -11.320 7.6 0.48 16.0 0.0 0.00 0.0
4U 1722-30 261.864 -30.810 1.8 356.302 +2.311 3.9 0.25 15.6 1.4 0.20 6.7
SAX J1810.8-2609 272.718 -26.154 2.0 5.208 -3.458 3.8 0.27 14.0 1.5 0.22 7.0
GX 9+1 270.404 -20.525 2.0 9.089 +1.140 4.6 0.34 13.6 0.0 0.00 0.0
4U 1700-377 255.949 -37.851 2.6 347.731 +2.192 5.1 0.50 10.1 0.0 0.00 0.0
GX 354-0 262.994 -33.839 2.5 354.301 -0.155 2.9 0.27 10.7 0.0 0.00 0.0
SLX 1744-299_300 266.809 -29.988 3.2 359.284 -0.847 1.7 0.21 8.1 0.0 0.00 0.0
IGR J17456-2901 266.417 -28.969 3.3 359.978 -0.026 1.6 0.21 7.7 0.0 0.00 0.0
H 1702-429 256.577 -43.039 3.7 343.890 -1.328 9.8 1.40 7.0 0.0 0.00 0.0
SAX J1712.6-3739 258.151 -37.653 3.4 348.931 +0.916 3.3 0.43 7.6 0.0 0.00 0.0
IGR J17091-3624 257.241 -36.426 3.7 349.490 +2.228 2.8 0.41 6.8 0.0 0.00 0.0
SLX 1735-269 264.568 -26.973 4.1 0.812 +2.414 1.4 0.24 6.1 1.1 0.20 5.6
GX 17+2 274.006 -14.056 4.3 16.415 +1.268 10.2 1.75 5.8 0.0 0.00 0.0
3A 1728-169 262.923 -16.932 4.5 8.533 +9.062 3.1 0.56 5.5 0.0 0.00 0.0
IGR J17544-2619 268.594 -26.337 5.7 3.226 -0.330 0.9 0.22 4.3 0.0 0.00 0.0
IGR J17498-2921 267.496 -29.324 4.3 0.161 -1.016 1.2 0.20 5.8 0.0 0.00 0.0
GRS 1734-292 264.313 -29.176 5.0 358.830 +1.426 1.1 0.22 5.0 0.0 0.00 0.0
1E 1743.1-2843 266.587 -28.674 0.0 0.307 -0.000 0.9 0.00 4.5 0.0 0.00 0.0
KS 1741-293 266.211 -29.415 0.0 359.503 -0.105 0.9 0.00 4.2 0.0 0.00 0.0
1A 1742-294 266.589 -29.497 0.0 359.604 -0.429 0.8 0.00 4.0 0.0 0.00 0.0
IGR J16500-3307 252.569 -33.045 6.2 349.799 +7.333 2.2 0.56 3.9 0.0 0.00 0.0
Swift J174444.9-2950 266.305 -29.827 0.0 359.195 -0.390 0.8 0.00 3.8 0.0 0.00 0.0
Swift J165441.9-4333 253.662 -43.471 6.5 342.242 +0.078 9.5 0.00 3.7 0.0 0.00 0.0
IGR J17252-3616 261.347 -36.261 6.5 351.537 -0.374 1.2 0.00 3.7 0.0 0.00 0.0
V2400 Oph 258.087 -24.251 7.1 359.828 +8.785 1.1 0.33 3.4 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 -29.515 359.559 -0.389 4.9 0.22 21.8 0.9 0.14 6.9
4U 1722-30 261.888 -30.802 356.320 +2.298 2.4 0.45 5.4 0.6 0.34 1.7
GX 3+1 266.993 -26.561 2.300 +0.788 40.6 0.41 99.0 4.5 0.21 21.9
GX 354-0 262.989 -33.835 354.302 -0.150 12.0 0.89 13.4 2.6 0.75 3.5
GX 5-1 270.284 -25.076 5.080 -1.017 125.0 1.61 77.4 14.0 0.71 19.9
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.22 9.6 0.3 0.14 2.4
NEW SOURCE 269.618 -24.587 5.204 -0.249 8.4 1.41 5.9 0.7 0.68 1.0
NEW SOURCE 267.788 -27.119 2.186 -0.108 1.8 0.31 5.7 0.2 0.18 1.1
NEW SOURCE 273.074 -26.440 5.109 -3.876 14.1 2.55 5.5 0.0 0.00 0.0
NEW SOURCE 267.555 -26.115 2.942 +0.586 2.4 0.45 5.4 0.0 0.00 0.0
NEW SOURCE 272.087 -27.407 3.836 -3.567 4.0 0.93 4.3 1.6 0.50 3.1
NEW SOURCE 262.100 -27.422 359.242 +4.015 1.4 0.44 3.1 0.8 0.30 2.7
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