Revolution 0424: Observation start 2006-04-03T16:51 = MJD 53828.703
Total Observation GTI = 12067 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 1700-377 255.984 -37.849 0.4 347.749 +2.172 100.5 0.83 121.2 27.3 0.61 44.7
GRS 1758-258 270.301 -25.737 1.0 4.513 -1.357 10.0 0.33 30.1 6.9 0.27 26.0
Ginga 1826-24 277.373 -23.793 1.0 9.278 -6.090 17.8 0.60 29.8 6.8 0.45 15.0
GX 5-1 270.283 -25.083 1.1 5.074 -1.020 10.0 0.38 26.4 0.0 0.00 0.0
GX 354-0 262.998 -33.823 1.1 354.316 -0.149 10.6 0.39 27.4 0.0 0.00 0.0
GX 1+4 263.004 -24.746 1.1 1.934 +4.799 10.3 0.37 27.9 0.0 0.00 0.0
H 1820-303 275.921 -30.373 1.5 2.779 -7.921 9.4 0.48 19.8 0.0 0.00 0.0
3A 1822-371 276.468 -37.124 2.5 356.841 -11.315 7.8 0.72 10.8 0.0 0.00 0.0
GX 349+2 256.401 -36.445 2.3 349.070 +2.757 7.4 0.63 11.7 0.0 0.00 0.0
4U 1722-30 261.891 -30.796 2.7 356.326 +2.300 3.7 0.37 9.9 1.9 0.29 6.5
SLX 1735-269 264.522 -27.014 3.0 0.756 +2.427 2.7 0.31 8.6 1.3 0.27 4.7
GX 9+1 270.381 -20.495 2.8 9.104 +1.174 4.4 0.47 9.3 0.0 0.00 0.0
XTE J1817-330 274.400 -33.011 3.4 359.812 -7.969 3.2 0.43 7.5 2.3 0.34 6.8
GX 3+1 266.979 -26.572 4.0 2.285 +0.792 2.3 0.36 6.4 0.0 0.00 0.0
GX 13+1 273.618 -17.148 3.8 13.519 +0.122 6.3 0.96 6.6 0.0 0.00 0.0
3A 1728-169 263.010 -17.004 4.8 8.516 +8.954 3.8 0.73 5.2 0.0 0.00 0.0
IGR J17541-2252 268.512 -22.811 4.2 6.230 +1.519 2.1 0.34 6.1 0.0 0.00 0.0
GX 17+2 273.951 -14.029 5.2 16.413 +1.328 12.9 2.71 4.8 0.0 0.00 0.0
SLX 1744-299_300 266.895 -30.060 4.6 359.261 -0.948 1.8 0.32 5.5 0.0 0.00 0.0
XTE J1710-281 257.483 -28.224 5.2 356.247 +6.917 2.1 0.00 4.7 0.0 0.00 0.0
1E 1742.8-2853 266.543 -28.920 5.9 0.077 -0.095 1.2 0.29 4.2 0.0 0.00 0.0
IGR J18193-2542 274.809 -25.817 4.7 6.397 -4.955 2.4 0.45 5.3 0.0 0.00 0.0
IGR J17488-3253 267.224 -32.860 6.7 357.005 -2.632 1.3 0.36 3.6 0.0 0.00 0.0
MAXI J1836-194 278.840 -19.272 6.0 13.949 -5.256 4.2 1.02 4.1 0.0 0.00 0.0
IGR J17195-4100 259.907 -41.058 6.8 346.947 -2.166 3.3 0.00 3.6 0.0 0.00 0.0
IGR J18135-1751 273.299 -17.818 6.7 12.784 +0.069 2.8 0.77 3.6 0.0 0.00 0.0
IGR J17454-2919 266.306 -29.420 0.0 359.542 -0.179 1.1 0.00 3.5 0.0 0.00 0.0
IGR J17597-2201 269.919 -21.929 7.0 7.646 +0.836 1.4 0.00 3.4 1.8 0.34 5.3
Swift J1753.7-2544 268.450 -25.666 5.7 3.739 +0.122 1.4 0.32 4.3 0.0 0.00 0.0
AX J1749.1-2733 267.302 -27.534 7.5 1.609 +0.050 1.0 0.30 3.2 0.0 0.00 0.0
1RXS J165443.5-19162 262.538 -19.267 0.0 6.339 +8.123 1.8 0.00 3.3 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 1742-294 266.522 -29.510 359.564 -0.386 3.1 0.30 10.2 0.8 0.17 4.8
1A 1743-288 266.760 -28.880 0.209 -0.236 8.3 0.33 25.4 0.8 0.18 4.6
GX 3+1 266.982 -26.570 2.287 +0.791 22.2 0.47 47.7 2.4 0.23 10.6
GX 354-0 262.980 -33.830 354.302 -0.141 16.7 1.17 14.2 3.7 0.83 4.4
GX 5-1 270.284 -25.079 5.077 -1.019 119.8 1.98 60.4 10.7 0.82 13.0
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.9 0.31 9.4 0.3 0.17 1.7
NEW SOURCE 267.595 -23.101 5.550 +2.098 11.4 2.41 4.7 1.5 1.35 1.1
NEW SOURCE 269.421 -24.152 5.491 +0.124 8.1 1.86 4.3 0.0 0.00 0.0
NEW SOURCE 268.029 -25.619 3.586 +0.473 2.9 0.65 4.5 0.4 0.32 1.3
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