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2004MNRAS.354..485B - Mon. Not. R. Astron. Soc., 354, 485-521 (2004/October-3)
The radio source population at high frequency: follow-up of the 15-GHz 9C survey.
BOLTON R.C., COTTER G., POOLEY G.G., RILEY J.M., WALDRAM E.M., CHANDLER C.J., MASON B.S., PEARSON T.J. and READHEAD A.C.S.
Abstract (from CDS):
Two flux-limited samples are defined, one containing 124 sources complete to 25 mJy and one of 70 sources complete to 60 mJy. Between one-fifth and one-quarter of sources from these flux-limited samples display convex radio spectra, rising between 1.4 and 4.8 GHz. These rising-spectrum sources make up a much larger fraction of the radio source population at this high selection frequency than in lower frequency surveys.
We find that by using non-simultaneous survey flux density measurements at 1.4 and 15 GHz to remove steep-spectrum objects, the efficiency of selecting objects with spectra rising between 1.4 and 4.8 GHz (as seen in simultaneous measurements) can be raised to 49 per cent without compromising the completeness of the rising-spectrum sample.
Abstract Copyright: 2004 RAS
Journal keyword(s): surveys - galaxies: active - radio continuum: general
VizieR on-line data: <Available at CDS (J/MNRAS/354/485): table2.dat>
Nomenclature: Table 2: [BCP2004] 9C JHHMM+DDMM N=51.
Simbad objects: 176
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