Revolution 0600: Observation start 2007-09-12T01:24 = MJD 54355.059
Total Observation GTI = 11475 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 1700-377 255.986 -37.846 0.6 347.753 +2.173 49.8 0.74 66.9 16.0 0.58 27.8
GX 1+4 263.011 -24.747 1.0 1.937 +4.793 13.1 0.43 30.2 0.0 0.00 0.0
Ginga 1826-24 277.373 -23.786 1.1 9.285 -6.087 18.4 0.65 28.4 8.6 0.51 17.0
GX 5-1 270.277 -25.084 1.3 5.070 -1.016 9.8 0.42 23.6 0.0 0.00 0.0
H 1820-303 275.926 -30.372 1.4 2.782 -7.924 10.0 0.48 20.7 0.0 0.00 0.0
GX 354-0 262.979 -33.839 1.4 354.294 -0.145 8.1 0.40 20.5 2.0 0.33 6.3
GX 349+2 256.464 -36.419 1.7 349.121 +2.733 11.2 0.67 16.7 0.0 0.00 0.0
GRS 1758-258 270.319 -25.706 2.4 4.548 -1.356 4.7 0.42 11.3 2.8 0.34 8.2
SAX J1810.8-2609 272.653 -26.184 2.1 5.153 -3.422 5.1 0.40 12.7 2.2 0.32 6.7
GX 17+2 274.013 -14.021 2.2 16.449 +1.279 34.8 2.83 12.3 0.0 0.00 0.0
3A 1822-371 276.469 -37.096 2.5 356.867 -11.304 7.8 0.72 10.7 0.0 0.00 0.0
GX 3+1 267.005 -26.576 2.9 2.293 +0.770 3.1 0.34 9.1 0.0 0.00 0.0
GX 9+1 270.452 -20.503 3.2 9.131 +1.111 4.0 0.50 8.1 0.0 0.00 0.0
4U 1722-30 261.873 -30.796 3.1 356.317 +2.312 3.2 0.39 8.3 1.6 0.32 5.2
3A 1728-169 262.996 -16.946 4.5 8.558 +8.996 4.1 0.73 5.5 0.0 0.00 0.0
H 1702-429 256.520 -42.988 4.6 343.906 -1.264 14.2 0.00 5.4 0.0 0.00 0.0
SLX 1744-299_300 266.815 -29.906 5.1 359.357 -0.809 1.5 0.32 4.8 0.0 0.00 0.0
1E 1743.1-2843 266.589 -28.756 0.0 0.238 -0.044 1.5 0.00 5.1 0.0 0.00 0.0
1A 1742-294 266.419 -29.441 4.3 359.575 -0.274 1.8 0.30 5.8 0.0 0.00 0.0
SLX 1735-269 264.499 -27.021 4.9 0.739 +2.440 1.8 0.35 5.1 1.8 0.29 6.0
SAX J1712.6-3739 258.185 -37.685 5.6 348.921 +0.875 2.8 0.64 4.4 0.0 0.00 0.0
Swift J174535.5-2901 266.307 -29.085 4.8 359.828 -0.005 1.5 0.30 5.2 0.0 0.00 0.0
IGR J17451-3022 266.342 -30.468 5.3 358.664 -0.752 1.5 0.33 4.7 0.0 0.00 0.0
AX J1749.2-2725 267.211 -27.456 5.3 1.634 +0.160 1.5 0.31 4.6 0.0 0.00 0.0
GRS 1734-292 264.375 -29.123 5.0 358.903 +1.408 1.6 0.32 5.0 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 1742-294 266.525 -29.546 359.533 -0.407 4.7 0.35 13.7 0.9 0.20 4.4
4U 1722-30 261.888 -30.802 356.320 +2.298 2.1 0.69 3.1 1.0 0.49 2.1
GRS 1758-258 270.303 -25.741 4.511 -1.361 3.8 1.22 3.1 1.1 0.57 2.0
GX 3+1 267.000 -26.565 2.300 +0.780 34.5 0.54 63.8 3.6 0.26 13.9
GX 354-0 262.989 -33.835 354.302 -0.150 5.4 1.38 3.9 0.0 0.00 0.0
GX 5-1 270.283 -25.082 5.074 -1.018 108.6 1.98 54.8 10.3 0.83 12.4
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.9 0.35 5.5 0.5 0.21 2.4
NEW SOURCE 268.197 -22.823 6.072 +1.763 20.1 3.46 5.8 3.2 1.80 1.8
NEW SOURCE 270.155 -26.187 4.057 -1.466 4.5 0.99 4.6 0.8 0.47 1.7
NEW SOURCE 269.357 -25.688 4.132 -0.595 5.1 0.97 5.3 0.6 0.46 1.3
NEW SOURCE 269.103 -26.997 2.885 -1.056 2.5 0.57 4.4 0.4 0.29 1.5
NEW SOURCE 271.201 -25.325 5.271 -1.862 9.6 2.12 4.5 1.3 1.11 1.2
NEW SOURCE 267.026 -25.390 3.319 +1.367 2.8 0.69 4.1 0.0 0.00 0.0
NEW SOURCE 272.308 -25.289 5.790 -2.719 14.1 4.04 3.5 0.0 0.00 0.0
NEW SOURCE 265.998 -23.755 4.231 +3.015 5.3 1.23 4.3 0.0 0.00 0.0
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