A 20 GHz Bright Sample for Delta > 72 deg - II. Multi-frequency Follow-up
arXiv:1307.8380 · doi:10.1093/mnras/stt1412
Abstract
We present follow-up observations at 5, 8 and 30 GHz of the K-band Northern Wide Survey (KNoWS) 20 GHz Bright Sample, performed with the 32-m Medicina Radio Telescope and the 32-m Torun Radio Telescope. The KNoWS sources were selected in the Northern Polar Cap (Delta > 72 deg) and have a flux density limit S(20GHz) = 115 mJy. We include NVSS 1.4 GHz measurements to derive the source radio spectra between 1.4 and 30 GHz. Based on optical identifications, 68 per cent of the sources are QSOs, and 27 per cent are radio galaxies. A redshift measurement is available for 58 per cent of the sources. The radio spectral properties of the different source populations are found to be in agreement with those of other high-frequency selected samples.
14 pages, 6 figures, 7 tables. Accepted for publication on MNRAS
References in corpus (7)
- The properties of extragalactic radio sources selected at 20 GHz
- Statistical analyses of long-term variability of AGN at high radio frequencies
- The Australia Telescope 20 GHz (AT20G) Survey: The Bright Source Sample
- 30 GHz flux density measurements of the Caltech-Jodrell flat-spectrum sources with OCRA-p
- Multi-frequency spectral analysis of extragalactic radio sources in the 33-GHz VSA catalogue: sources with flattening and upturn spectrum
- The Planck-ATCA Co-eval Observations (PACO) project: the spectrally-selected sample
- VLA/JVLA Monitoring of Bright Northern Radio Sources
Cited by in corpus (4)
- The Sardinia Radio Telescope: From a Technological Project to a Radio Observatory
- A Broadband Polarization Catalog of Extragalactic Radio Sources
- Parsec-scale properties of steep and flat spectrum extragalactic radio sources from a VLBA survey of a complete north polar cap sample
- The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region