Revolution 1854: Observation start 2017-08-24T20:46 = MJD 57989.866
Total Observation GTI = 12499 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 1700-377 255.990 -37.868 0.7 347.738 +2.157 73.6 1.45 50.7 14.1 0.60 23.4
IGR J17464-3213 266.567 -32.234 0.8 357.256 -1.835 24.0 0.60 40.2 11.3 0.28 40.4
1E 1740.7-2942 265.984 -29.753 0.9 359.111 -0.114 21.4 0.58 36.8 9.7 0.27 35.9
GRS 1758-258 270.315 -25.744 1.1 4.513 -1.372 16.2 0.60 26.7 7.0 0.28 25.1
GRS 1716-249 259.878 -25.036 1.5 0.114 +7.000 17.6 0.95 18.5 7.4 0.41 18.1
OAO 1657-415 255.248 -41.646 1.8 344.397 +0.299 44.2 2.90 15.2 12.4 1.16 10.7
SLX 1735-269 264.590 -26.973 2.7 0.823 +2.397 6.1 0.62 9.8 1.8 0.28 6.4
GX 5-1 270.344 -25.063 2.6 5.118 -1.058 6.3 0.61 10.3 0.0 0.00 0.0
GX 1+4 263.015 -24.742 2.9 1.943 +4.792 6.6 0.74 8.9 0.0 0.00 0.0
3A 1822-371 276.428 -37.104 3.4 356.845 -11.278 8.8 1.17 7.5 0.0 0.00 0.0
GX 9+1 270.302 -20.531 4.1 9.037 +1.220 5.5 0.90 6.1 0.0 0.00 0.0
AX J1820.5-1434 275.150 -14.510 4.0 16.540 +0.077 20.8 3.27 6.4 0.0 0.00 0.0
MXB 1730-335 263.241 -33.373 4.3 354.804 -0.074 4.0 0.00 5.8 0.0 0.00 0.0
1A 1743-288 266.718 -28.880 4.2 0.191 -0.205 3.6 0.60 6.0 0.0 0.00 0.0
SLX 1744-299_300 266.896 -30.074 5.2 359.249 -0.956 2.8 0.58 4.7 1.2 0.00 4.3
GX 349+2 256.450 -36.447 4.7 349.091 +2.725 7.4 1.40 5.3 0.0 0.00 0.0
Oph Cluster 258.171 -23.276 5.1 0.681 +9.282 4.6 0.95 4.8 0.0 0.00 0.0
GX 17+2 274.030 -13.950 4.5 16.519 +1.298 28.0 4.99 5.6 0.0 0.00 0.0
1RXS J170849.0-40091 257.073 -40.152 4.9 346.422 +0.108 9.1 1.82 5.0 0.0 0.00 0.0
IGR J18027-1455 270.780 -14.950 5.2 14.123 +3.572 13.6 0.00 4.8 0.0 0.00 0.0
4U 1708-40 258.126 -40.814 4.5 346.364 -0.929 9.9 1.79 5.5 0.0 0.00 0.0
GRS 1734-292 264.342 -29.050 0.0 358.949 +1.471 2.7 0.00 4.4 0.0 0.00 0.0
GX 354-0 263.029 -33.775 0.0 354.370 -0.145 3.1 0.00 4.4 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 -29.501 359.572 -0.382 6.6 0.22 29.6 0.4 0.14 2.5
1E 1740.7-2942 265.978 -29.745 359.116 -0.106 3.2 0.23 13.8 1.3 0.15 8.8
4U 1722-30 261.888 -30.802 356.320 +2.298 6.9 0.54 12.7 0.5 0.40 1.3
GX 3+1 266.985 -26.573 2.287 +0.788 29.6 0.37 79.5 1.3 0.21 6.4
GX 354-0 262.989 -33.835 354.302 -0.150 16.7 1.03 16.2 1.1 0.77 1.4
GX 5-1 270.285 -25.091 5.068 -1.025 97.3 1.21 80.7 4.2 0.56 7.6
IGR J17464-3213 266.567 -32.229 357.260 -1.832 3.7 0.28 13.0 1.6 0.20 7.8
MXB 1730-335 263.350 -33.388 354.841 -0.158 9.8 0.77 12.8 0.9 0.55 1.6
SLX 1735-269 264.571 -26.994 0.796 +2.400 1.2 0.35 3.3 0.4 0.23 1.9
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 1.2 0.22 5.8 0.4 0.14 2.6
1A 1743-288 266.773 -28.887 0.210 -0.250 1.2 0.23 5.4 0.3 0.15 1.9
NEW SOURCE 266.876 -23.744 4.659 +2.334 5.6 1.22 4.6 0.0 0.00 0.0
NEW SOURCE 270.150 -24.845 5.221 -0.797 6.1 1.13 5.4 0.9 0.59 1.6
NEW SOURCE 272.892 -27.329 4.248 -4.157 3.9 1.01 3.9 0.0 0.00 0.0
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