Revolution 0657: Observation start 2008-02-29T13:05 = MJD 54525.546
Total Observation GTI = 10024 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRO J1750-27 267.298 -26.647 0.4 2.368 +0.510 42.6 0.39 109.7 1.9 0.32 6.1
4U 1700-377 255.984 -37.838 0.9 347.758 +2.179 32.0 0.85 37.8 9.5 0.64 15.0
Ginga 1826-24 277.358 -23.788 1.0 9.277 -6.076 19.2 0.65 29.6 7.9 0.49 16.3
4U 1722-30 261.886 -30.808 1.3 356.314 +2.296 9.4 0.41 22.7 3.1 0.32 9.7
H 1820-303 275.911 -30.367 1.5 2.780 -7.911 10.9 0.57 19.1 0.0 0.00 0.0
GX 3+1 266.972 -26.543 0.0 2.306 +0.813 5.1 0.00 12.9 0.0 0.00 0.0
GX 9+1 270.357 -20.525 3.0 9.067 +1.178 4.8 0.56 8.7 0.0 0.00 0.0
1E 1740.7-2942 265.958 -29.726 3.3 359.123 -0.081 2.9 0.36 7.9 2.5 0.31 8.0
GRS 1758-258 270.307 -25.720 2.6 4.531 -1.354 4.2 0.42 10.1 2.6 0.33 7.8
GX 349+2 256.428 -36.454 3.1 349.076 +2.734 6.2 0.74 8.5 0.0 0.00 0.0
GX 354-0 263.009 -33.756 3.5 354.377 -0.120 3.2 0.44 7.3 0.0 0.00 0.0
3A 1822-371 276.487 -37.072 3.3 356.896 -11.307 5.7 0.73 7.9 0.0 0.00 0.0
SLX 1735-269 264.534 -26.976 4.1 0.794 +2.438 2.5 0.40 6.2 0.0 0.00 0.0
GX 17+2 274.002 -14.069 3.9 16.401 +1.265 24.7 3.86 6.4 0.0 0.00 0.0
SLX 1744-299_300 266.792 -30.076 5.4 359.201 -0.880 1.6 0.36 4.6 0.0 0.00 0.0
1A 1742-294 266.496 -29.584 0.0 359.488 -0.405 2.0 0.00 5.8 0.0 0.00 0.0
GX 1+4 262.987 -24.735 5.0 1.935 +4.818 2.4 0.49 5.0 0.0 0.00 0.0
MXB 1730-335 263.234 -33.386 0.0 354.789 -0.076 2.3 0.00 5.3 0.0 0.00 0.0
GX 5-1 270.305 -25.119 5.0 5.052 -1.054 2.1 0.43 4.9 0.0 0.00 0.0
IGR J17404-3655 265.126 -36.929 5.9 352.630 -3.283 2.3 0.00 4.2 0.0 0.00 0.0
SLX 1737-282 265.288 -28.340 6.0 359.993 +1.147 1.5 0.00 4.1 0.0 0.00 0.0
IGR J17252-3616 261.238 -36.312 5.4 351.446 -0.331 2.5 0.54 4.6 0.0 0.00 0.0
MAXI J1659-152 254.718 -15.228 6.7 5.518 +16.574 14.5 4.05 3.6 0.0 0.00 0.0
H 1702-429 256.569 -43.089 5.2 343.847 -1.353 10.2 2.16 4.7 0.0 0.00 0.0
1E 1742.8-2853 266.597 -29.000 7.4 0.033 -0.176 1.1 0.35 3.2 0.0 0.00 0.0
IGR J17375-3022 264.397 -30.299 5.9 357.921 +0.762 1.5 0.36 4.1 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 1.8 0.38 4.7 0.5 0.23 2.1
4U 1722-30 261.888 -30.802 356.320 +2.298 2.9 0.77 3.8 1.3 0.57 2.3
GRO J1750-27 267.319 -26.642 2.382 +0.496 17.3 0.66 26.1 10.7 0.38 28.4
GX 3+1 266.984 -26.561 2.296 +0.794 44.4 0.71 62.8 4.6 0.36 12.8
GX 354-0 262.989 -33.835 354.302 -0.150 8.9 1.39 6.4 1.2 1.04 1.2
GX 5-1 270.282 -25.080 5.075 -1.018 87.1 2.24 38.8 4.6 1.02 4.5
MXB 1730-335 263.350 -33.388 354.841 -0.158 10.7 1.12 9.6 0.8 0.73 1.1
SLX 1737-282 265.163 -28.297 359.971 +1.264 1.3 0.43 3.1 0.3 0.26 1.2
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.5 0.37 6.7 0.5 0.23 2.2
SLX 1746-331 267.467 -33.195 356.822 -2.979 3.4 0.60 5.7 0.0 0.00 0.0
NEW SOURCE 266.475 -22.851 5.232 +3.111 18.6 4.15 4.5 4.4 2.81 1.6
NEW SOURCE 264.343 -25.450 1.994 +3.398 4.7 1.10 4.2 0.0 0.00 0.0
NEW SOURCE 268.279 -26.783 2.699 -0.313 2.4 0.63 3.8 0.4 0.35 1.3
NEW SOURCE 265.462 -24.852 3.040 +2.856 4.4 1.16 3.8 0.0 0.00 0.0
NEW SOURCE 266.415 -23.798 4.393 +2.667 7.0 1.97 3.6 0.0 0.00 0.0
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