Revolution 1404: Observation start 1999-12-31T23:58 = MJD 51544
Total Observation GTI = 10373 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 J1744-28 266.138 -28.742 0.3 0.044 +0.301 79.7 0.38 209.4 9.3 0.24 38.4
GRS 1739-278 265.666 -27.745 0.6 0.674 +1.178 29.1 0.43 67.9 8.4 0.27 30.9
GX 1+4 263.016 -24.745 1.1 1.941 +4.790 12.7 0.44 28.8 0.0 0.00 0.0
Ginga 1826-24 277.339 -23.774 1.1 9.281 -6.054 21.1 0.79 26.7 9.4 0.46 20.5
GRS 1758-258 270.315 -25.724 1.2 4.531 -1.362 11.5 0.45 25.7 8.8 0.27 32.5
GX 5-1 270.288 -25.088 1.5 5.071 -1.026 8.9 0.48 18.7 0.0 0.00 0.0
GX 349+2 256.435 -36.439 2.2 349.091 +2.739 8.9 0.73 12.2 0.0 0.00 0.0
OAO 1657-415 255.218 -41.585 3.3 344.431 +0.355 17.4 2.22 7.9 0.0 0.00 0.0
H 1820-303 275.936 -30.370 3.0 2.787 -7.931 5.6 0.65 8.7 0.0 0.00 0.0
SLX 1735-269 264.512 -26.974 3.2 0.785 +2.456 3.3 0.41 8.0 1.6 0.26 6.3
GX 354-0 262.976 -33.822 3.3 354.307 -0.134 3.7 0.47 7.8 0.0 0.00 0.0
GX 3+1 267.003 -26.569 3.4 2.299 +0.776 3.3 0.43 7.5 0.0 0.00 0.0
4U 1722-30 261.890 -30.840 3.5 356.289 +2.276 3.5 0.48 7.3 1.3 0.29 4.7
3A 1822-371 276.460 -37.179 3.7 356.788 -11.333 6.0 0.88 6.9 0.0 0.00 0.0
1E 1740.7-2942 265.980 -29.767 0.0 359.099 -0.118 2.6 0.00 6.7 0.0 0.00 0.0
IGR J18027-1455 270.648 -14.914 4.3 14.092 +3.701 10.8 1.84 5.9 0.0 0.00 0.0
IGR J17494-3030 267.348 -30.578 5.2 359.019 -1.550 1.9 0.41 4.7 0.0 0.00 0.0
SAX J1810.8-2609 272.769 -26.140 0.0 5.243 -3.492 2.4 0.00 4.8 0.0 0.00 0.0
MAXI J1836-194 278.969 -19.354 3.9 13.931 -5.402 9.9 1.53 6.5 0.0 0.00 0.0
XTE J1719-291 259.914 -29.000 4.8 356.848 +4.727 2.6 0.52 5.1 0.0 0.00 0.0
XTE J1710-281 257.464 -28.129 4.9 356.314 +6.986 2.9 0.57 5.1 0.0 0.00 0.0
IGR J17252-3616 261.391 -36.273 5.4 351.547 -0.411 2.6 0.58 4.5 0.0 0.00 0.0
XMMSL1 J171900.4-353 259.766 -35.607 5.7 351.349 +1.050 2.5 0.00 4.3 0.0 0.00 0.0
IGR J17407-2808 265.233 -28.154 0.0 0.125 +1.287 1.8 0.00 4.2 0.0 0.00 0.0
1E 1742.9-2849 266.575 -28.907 0.0 0.103 -0.112 1.7 0.00 4.1 0.0 0.00 0.0
Swift J175648.6-2544 269.238 -25.852 5.9 3.936 -0.585 2.0 0.00 4.1 0.0 0.00 0.0
GRS 1734-292 264.283 -29.122 0.0 358.861 +1.476 1.6 0.00 4.0 0.0 0.00 0.0
NEW SOURCE 268.396 -24.280 4.5 4.908 +0.867 2.4 0.43 5.6 0.0 0.00 0.0
NEW SOURCE 260.056 -37.920 4.4 349.587 -0.465 3.5 0.62 5.7 0.0 0.00 0.0
NEW SOURCE 253.201 -28.701 3.8 353.567 +9.631 5.7 0.85 6.6 0.0 0.00 0.0
NEW SOURCE 278.679 -24.180 4.1 9.471 -7.330 6.4 1.05 6.1 0.0 0.00 0.0
NEW SOURCE 273.865 -27.036 4.6 4.919 -4.780 2.8 0.52 5.4 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 -29.515 359.559 -0.389 9.8 0.34 28.3 1.3 0.18 7.1
4U 1722-30 261.888 -30.802 356.320 +2.298 2.3 0.65 3.5 1.0 0.39 2.5
GRO J1744-28 266.141 -28.741 0.045 +0.299 43.2 0.38 114.7 20.8 0.20 102.1
GRS 1739-278 265.668 -27.748 0.673 +1.175 42.0 0.42 100.7 7.9 0.21 38.7
GX 1+4 263.009 -24.746 1.937 +4.795 5.1 1.14 4.5 2.4 0.60 3.9
GX 3+1 266.979 -26.561 2.293 +0.798 49.1 0.52 94.8 3.8 0.24 15.4
GX 354-0 262.989 -33.835 354.302 -0.150 23.1 1.29 17.9 3.4 0.85 4.0
GX 5-1 270.284 -25.079 5.077 -1.019 169.1 2.86 59.2 15.4 1.25 12.3
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.1 0.33 6.3 0.0 0.00 0.0
NEW SOURCE 271.017 -25.573 4.974 -1.838 18.4 3.21 5.7 3.0 1.95 1.5
NEW SOURCE 270.225 -25.714 4.499 -1.286 7.2 1.55 4.7 0.0 0.00 0.0
NEW SOURCE 269.007 -27.372 2.518 -1.170 2.8 0.55 5.0 0.3 0.29 1.2
NEW SOURCE 269.436 -23.447 6.108 +0.465 13.8 3.07 4.5 0.0 0.00 0.0
NEW SOURCE 269.781 -25.582 4.415 -0.874 6.0 1.34 4.5 0.0 0.00 0.0
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