The CLASS blazar survey. III. (Caccianiga+, 2004)

Details The CLASS blazar survey. III. (Caccianiga+, 2004) The CLASS blazar survey. III. (Caccianiga+, 2004)

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..73480937c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/348/937. Originally published in: 2004MNRAS.348..937C

Physics

Bl Lac Objects, Qsos, Radio Sources

Scientific paper

We discuss the properties of the sources in the CLASS blazar survey, which aims at the selection of low radio power (P5GHz<1025W/Hz) blazars. We use Very Large Array (VLA) data from available catalogues and from our own observations to constrain the radio core-dominance of the sample which, together with the flat radio spectral index, is a signature of the blazar activity. X-ray data from the ROSAT All Sky Survey were also collected in order to constrain the radio-to-X-ray luminosity ratio of the sources.
(1 data file).

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