Revolution 0673: Observation start 2008-04-17T09:35 = MJD 54573.4
Total Observation GTI = 10696 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
==================== ======== ======= === ======== ======== ====== ===== ===== ====== ===== =====
IGR J17473-2721 266.827 -27.346 0.4 1.552 +0.508 54.4 0.40 137.2 22.8 0.31 73.4
4U 1700-377 255.986 -37.850 0.7 347.750 +2.170 46.8 0.93 50.5 13.6 0.67 20.4
GX 5-1 270.292 -25.083 0.8 5.077 -1.026 19.4 0.44 44.4 0.0 0.00 0.0
GRO J1750-27 267.254 -26.638 1.0 2.355 +0.548 13.0 0.40 32.8 0.0 0.00 0.0
GX 354-0 262.987 -33.837 1.1 354.299 -0.150 13.1 0.45 29.2 3.5 0.34 10.4
SAX J1750.8-2900 267.607 -29.035 1.1 0.459 -0.951 10.2 0.38 26.7 4.3 0.30 14.3
Ginga 1826-24 277.372 -23.800 1.2 9.272 -6.093 17.3 0.71 24.4 7.3 0.50 14.7
H 1820-303 275.905 -30.372 1.5 2.773 -7.908 10.4 0.53 19.5 0.0 0.00 0.0
GRS 1758-258 270.312 -25.739 1.7 4.516 -1.367 7.2 0.44 16.2 4.3 0.34 12.9
4U 1722-30 261.872 -30.789 1.8 356.323 +2.317 7.5 0.48 15.7 3.0 0.37 8.1
GX 9+1 270.395 -20.496 2.5 9.110 +1.162 6.0 0.55 10.9 0.0 0.00 0.0
GX 3+1 266.904 -26.504 2.5 2.308 +0.885 4.1 0.00 10.8 0.0 0.00 0.0
1E 1740.7-2942 265.958 -29.734 2.9 359.116 -0.085 3.5 0.39 9.2 3.4 0.30 11.2
XTE J1810-189 272.594 -19.076 2.7 11.360 +0.050 7.4 0.76 9.7 3.2 0.56 5.6
GX 349+2 256.433 -36.423 3.3 349.103 +2.750 6.5 0.85 7.7 0.0 0.00 0.0
3A 1822-371 276.390 -37.098 3.5 356.837 -11.248 5.4 0.73 7.4 0.0 0.00 0.0
3A 1728-169 262.944 -16.984 3.9 8.499 +9.017 5.9 0.91 6.5 0.0 0.00 0.0
IGR J17456-2901 266.413 -29.001 3.9 359.948 -0.040 2.5 0.39 6.4 0.0 0.00 0.0
SLX 1744-299_300 266.869 -29.949 6.6 359.344 -0.871 1.3 0.37 3.7 0.0 0.00 0.0
XTE J1709-267 257.363 -26.726 5.5 357.408 +7.881 2.6 0.59 4.5 1.9 0.42 4.5
GX 1+4 262.970 -24.717 5.6 1.941 +4.840 1.8 0.41 4.4 0.0 0.00 0.0
GX 17+2 274.017 -14.024 5.2 16.448 +1.274 14.3 3.04 4.7 0.0 0.00 0.0
GX 13+1 273.649 -17.167 5.8 13.516 +0.087 4.4 0.00 4.2 0.0 0.00 0.0
NEW SOURCE 253.927 -24.001 4.2 357.754 +11.997 5.6 0.94 5.9 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 1742-294 266.518 -29.515 359.557 -0.386 3.9 0.36 10.7 0.9 0.22 4.1
4U 1722-30 261.888 -30.802 356.320 +2.298 4.0 0.85 4.6 1.4 0.62 2.2
GRS 1747-312 267.690 -31.292 358.555 -2.168 1.3 0.41 3.1 0.0 0.00 0.0
GRS 1758-258 270.303 -25.741 4.511 -1.361 4.3 1.20 3.6 0.9 0.59 1.5
GX 3+1 266.991 -26.551 2.308 +0.794 38.7 0.61 63.2 4.8 0.32 15.1
GX 354-0 262.989 -33.835 354.302 -0.150 5.8 1.51 3.8 2.3 1.41 1.6
GX 5-1 270.294 -25.083 5.078 -1.028 125.8 1.86 67.7 17.2 0.83 20.8
IGR J17473-2721 266.830 -27.342 1.557 +0.508 15.3 0.47 32.3 7.6 0.27 27.8
SAX J1750.8-2900 267.594 -29.024 0.462 -0.936 3.6 0.38 9.5 1.2 0.23 5.5
SLX 1744-299_300 266.858 -29.999 359.297 -0.889 2.0 0.35 5.6 0.5 0.21 2.3
GRO J1750-27 267.300 -26.641 2.373 +0.511 3.5 0.55 6.4 2.6 0.31 8.6
NEW SOURCE 273.507 -26.901 4.887 -4.435 15.0 3.79 4.0 0.0 0.00 0.0
NEW SOURCE 273.034 -26.688 4.874 -3.963 10.8 2.40 4.5 0.0 0.00 0.0
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