Astron. Astrophys. Suppl. Ser. 143, 303-333
C. De Breuck1,2 -
W. van Breugel2 -
H.J.A. Röttgering1 -
Send offprint request: C. De Breuck
1 - Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands
2 - Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, L-413, Livermore, CA 94550, U.S.A.
Received November 4, 1999; accepted February 4, 2000
Comparison with spectrally unbiased samples at similar flux density levels, shows that our spectral index, flux density, and angular size selections do not affect the angular size distribution of the sample, but do avoid significant contributions by faint foreground spiral galaxies. We find that the spectral index distribution of 143000 sources from the WENSS and NVSS consists of a steep spectrum galaxy and a flat spectrum quasar population, with the relative contribution of flat spectrum sources doubling from S1400>0.1 Jy to S1400>2.5 Jy. The identification fraction of our USS sources on the POSS ( ) is as low as 15%, independent of spectral index . We further show that 85% of the USS sources that can be identified with an X-ray source are probably contained in galaxy clusters, and that sources are excellent Galactic pulsar candidates, because the percentage of these sources is four times higher in the Galactic plane.
Our sample has been constructed to start an intensive campaign to obtain a large sample of high redshift objects (z>3) that is selected in a way that does not suffer from dust extinction or any other optical bias.
Key words: surveys -- galaxies: active -- radio continuum: galaxies
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