Revolution 1597: Observation start 2015-10-11T05:57 = MJD 57306.248
Total Observation GTI = 16401 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 1758-258 270.305 -25.740 0.9 4.512 -1.362 12.0 0.34 34.7 9.8 0.22 44.2
SAX J1750.8-2900 267.621 -29.037 1.5 0.463 -0.963 5.7 0.31 18.7 2.5 0.20 12.1
H 1820-303 275.925 -30.372 1.7 2.781 -7.923 8.2 0.48 16.9 2.4 0.30 8.0
1E 1740.7-2942 265.982 -29.746 1.8 359.117 -0.109 5.4 0.36 15.2 4.8 0.23 20.4
GX 1+4 263.004 -24.747 2.2 1.933 +4.798 4.7 0.38 12.4 0.0 0.00 0.0
OAO 1657-415 255.203 -41.680 2.8 344.350 +0.305 16.9 1.77 9.5 0.0 0.00 0.0
GX 349+2 256.447 -36.435 3.0 349.100 +2.734 5.6 0.65 8.7 0.0 0.00 0.0
3A 1822-371 276.384 -37.089 3.0 356.844 -11.240 5.6 0.65 8.6 1.8 0.00 4.5
GX 9+1 270.380 -20.507 3.2 9.094 +1.168 3.8 0.48 8.0 0.0 0.00 0.0
GRS 1739-278 265.697 -27.794 3.2 0.647 +1.128 2.4 0.30 8.1 1.7 0.20 8.5
GX 17+2 273.938 -13.980 3.0 16.450 +1.362 27.0 3.14 8.6 0.0 0.00 0.0
SAX J1806.5-2215 271.603 -22.287 0.0 8.103 -0.698 3.3 0.00 7.5 2.0 0.28 7.0
GX 354-0 262.961 -33.904 4.1 354.231 -0.168 2.1 0.34 6.2 0.0 0.00 0.0
SLX 1744-299_300 266.786 -29.975 3.7 359.285 -0.823 2.2 0.33 6.8 0.0 0.00 0.0
IGR J17088-4008 257.184 -40.135 5.0 0.000 +0.000 4.3 0.88 4.9 0.0 0.00 0.0
MXB 1730-335 263.382 -33.388 4.7 354.855 -0.181 1.9 0.37 5.3 0.0 0.00 0.0
H 1702-429 256.627 -43.000 4.8 0.000 +0.000 11.6 0.00 5.2 0.0 0.00 0.0
IGR J18027-2016 270.733 -20.295 0.0 9.441 +0.985 2.4 0.00 5.0 0.0 0.00 0.0
IGR J18245-2452 276.166 -24.950 4.9 7.739 -5.641 2.8 0.56 5.1 0.0 0.00 0.0
GX 5-1 270.274 -25.033 5.0 5.113 -0.987 1.8 0.35 4.9 0.0 0.00 0.0
4U 1722-30 261.874 -30.739 4.4 356.366 +2.343 2.1 0.37 5.6 0.0 0.00 0.0
IGR J16558-4150 253.923 -41.730 0.0 343.717 +1.023 8.8 0.00 4.5 0.0 0.00 0.0
SLX 1735-269 264.464 -27.019 0.0 0.724 +2.468 1.5 0.00 4.4 1.3 0.21 6.3
1A 1742-294 266.497 -29.500 0.0 359.560 -0.362 1.5 0.00 4.4 0.0 0.00 0.0
GRS 1734-292 264.257 -29.123 4.5 358.848 +1.496 1.7 0.31 5.5 0.0 0.00 0.0
JEM-X
JEM-X1+2 combined 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+2 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 5.7 0.17 32.8 1.8 0.13 14.2
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 1.0 0.17 5.8 0.8 0.12 6.8
1E 1743.1-2843 266.587 -28.729 0.260 -0.029 0.9 0.17 4.9 0.4 0.12 3.5
4U 1722-30 261.888 -30.802 356.320 +2.298 6.7 0.34 19.9 1.4 0.26 5.3
GRS 1734-292 264.367 -29.142 358.883 +1.404 0.9 0.18 5.0 0.2 0.12 1.9
GRS 1758-258 270.303 -25.741 4.511 -1.361 1.6 0.71 2.3 1.6 0.46 3.4
GX 3+1 266.978 -26.558 2.297 +0.801 28.2 0.29 97.9 3.7 0.17 22.2
GX 354-0 262.989 -33.835 354.302 -0.150 11.6 0.71 16.3 5.4 0.69 7.8
GX 5-1 270.280 -25.083 5.072 -1.017 76.8 1.17 65.6 8.7 0.64 13.5
MXB 1730-335 263.356 -33.393 354.839 -0.165 9.3 0.50 18.6 3.6 0.43 8.4
SLX 1735-269 264.571 -26.994 0.796 +2.400 2.0 0.22 9.5 0.5 0.14 3.2
SLX 1737-282 265.163 -28.297 359.971 +1.264 0.6 0.17 3.3 0.0 0.00 0.0
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.1 0.17 6.2 0.6 0.13 4.9
Swift J174535.5-2901 266.398 -29.026 359.920 -0.042 1.0 0.17 5.7 0.7 0.12 5.3
SAX J1750.8-2900 267.608 -29.039 0.456 -0.954 1.9 0.19 10.0 0.9 0.14 6.2
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