Revolution 0295: Observation start 2005-03-15T04:03 = MJD 53444.169
Total Observation GTI = 13240 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
GRS 1758-258 270.308 -25.736 0.8 4.517 -1.362 12.3 0.28 43.4 8.1 0.23 35.4
Ginga 1826-24 277.360 -23.788 1.0 9.277 -6.078 16.6 0.51 32.8 5.3 0.39 13.5
1E 1740.7-2942 265.974 -29.743 0.9 359.115 -0.101 9.1 0.26 34.4 5.2 0.22 23.6
4U 1700-377 256.002 -37.839 1.1 347.766 +2.167 18.6 0.67 27.7 6.3 0.52 12.2
GX 349+2 256.441 -36.411 1.1 349.116 +2.752 13.8 0.52 26.4 0.0 0.00 0.0
GRO J1655-40 253.483 -39.843 1.3 344.975 +2.468 23.3 1.03 22.7 12.4 0.76 16.2
OAO 1657-415 255.208 -41.645 1.4 344.379 +0.323 26.6 1.25 21.3 6.4 0.97 6.6
IGR J17252-3616 261.308 -36.279 1.5 351.505 -0.359 7.6 0.40 19.2 0.0 0.00 0.0
4U 1722-30 261.902 -30.799 1.9 356.329 +2.290 4.6 0.31 14.9 1.7 0.25 7.0
GX 354-0 262.996 -33.825 2.0 354.314 -0.149 4.8 0.35 13.8 0.0 0.00 0.0
1A 1742-294 266.498 -29.519 2.4 359.545 -0.373 3.0 0.27 11.2 0.0 0.00 0.0
H 1820-303 275.904 -30.379 2.2 2.766 -7.911 5.4 0.44 12.3 0.0 0.00 0.0
3A 1822-371 276.452 -37.062 2.7 356.892 -11.277 5.6 0.58 9.6 0.0 0.00 0.0
GX 3+1 267.007 -26.530 3.9 2.334 +0.793 1.9 0.29 6.6 0.0 0.00 0.0
GX 5-1 270.259 -25.089 3.3 5.058 -1.003 2.3 0.30 7.9 0.0 0.00 0.0
SLX 1735-269 264.513 -26.988 4.1 0.774 +2.448 1.9 0.31 6.1 1.4 0.26 5.6
GX 9+1 270.421 -20.509 3.7 9.111 +1.133 2.8 0.41 6.8 0.0 0.00 0.0
1E 1742.9-2849 266.607 -28.879 4.6 0.141 -0.121 1.4 0.26 5.4 0.0 0.00 0.0
3A 1728-169 262.925 -16.930 4.1 8.535 +9.062 4.1 0.67 6.1 0.0 0.00 0.0
SLX 1744-299_300 266.922 -30.016 5.5 359.311 -0.945 1.3 0.30 4.5 0.0 0.00 0.0
SAX J1712.6-3739 258.176 -37.724 4.8 348.886 +0.858 2.4 0.47 5.2 0.0 0.00 0.0
1H 1746-370 267.476 -37.062 6.1 353.491 -4.957 1.7 0.41 4.0 0.0 0.00 0.0
IGR J17473-2721 266.764 -27.417 6.3 1.462 +0.519 1.2 0.31 3.8 0.0 0.00 0.0
4U 1735-444 264.693 -44.490 5.9 346.001 -6.985 12.1 2.96 4.1 0.0 0.00 0.0
IGR J18048-1455 271.288 -14.861 6.8 14.441 +3.188 5.0 0.00 3.5 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 2.1 0.20 10.2 0.8 0.12 6.9
1E 1740.7-2942 266.000 -29.747 359.124 -0.123 1.6 0.20 8.1 1.1 0.13 8.6
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.21 4.2 0.2 0.12 1.8
4U 1722-30 261.893 -30.798 356.325 +2.297 2.8 0.38 7.5 1.0 0.26 3.9
GRS 1741.9-2853 266.260 -28.914 359.953 +0.120 0.9 0.21 4.5 0.2 0.12 1.3
GRS 1758-258 270.303 -25.741 4.511 -1.361 5.1 0.87 5.9 1.3 0.43 3.0
GX 3+1 266.983 -26.559 2.298 +0.797 26.8 0.34 78.0 3.0 0.17 17.6
GX 354-0 263.004 -33.822 354.320 -0.153 13.9 0.84 16.5 3.5 0.60 5.9
GX 5-1 270.299 -25.072 5.090 -1.026 88.1 1.57 56.3 4.6 0.65 7.1
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.4 0.21 11.1 0.6 0.13 4.4
NEW SOURCE 267.880 -23.829 5.057 +1.502 5.8 1.08 5.4 0.6 0.56 1.0
NEW SOURCE 271.704 -25.798 5.079 -2.488 9.1 2.07 4.4 0.0 0.00 0.0
NEW SOURCE 269.934 -25.342 4.691 -0.874 4.3 1.05 4.0 0.0 0.00 0.0
NEW SOURCE 272.724 -27.877 3.694 -4.288 5.8 1.24 4.7 0.0 0.00 0.0
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