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 Toruń radio telescope. The KNoWS sources were selected in the Northern Polar Cap (δ > 72°) and have a flux density limit S20 GHz = 115 mJy. We include NRAO-VLA Sky Survey 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 quasars 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.

A 20 GHz bright sample for δ > 72° - II. Multifrequency follow-up / Ricci R.; Righini S.; Verma R.; Prandoni I.; Carretti E.; Mack K.-H.; Massardi M.; Procopio P.; Zanichelli A.; Gregorini L.; Mantovani F.; Gawroński M. P.; Peel M. W.. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 0035-8711. - STAMPA. - 435:(2013), pp. 2793-2805. [10.1093/mnras/stt1412]

A 20 GHz bright sample for δ > 72° - II. Multifrequency follow-up

GREGORINI, LORETTA;
2013

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 Toruń radio telescope. The KNoWS sources were selected in the Northern Polar Cap (δ > 72°) and have a flux density limit S20 GHz = 115 mJy. We include NRAO-VLA Sky Survey 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 quasars 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.
2013
A 20 GHz bright sample for δ > 72° - II. Multifrequency follow-up / Ricci R.; Righini S.; Verma R.; Prandoni I.; Carretti E.; Mack K.-H.; Massardi M.; Procopio P.; Zanichelli A.; Gregorini L.; Mantovani F.; Gawroński M. P.; Peel M. W.. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 0035-8711. - STAMPA. - 435:(2013), pp. 2793-2805. [10.1093/mnras/stt1412]
Ricci R.; Righini S.; Verma R.; Prandoni I.; Carretti E.; Mack K.-H.; Massardi M.; Procopio P.; Zanichelli A.; Gregorini L.; Mantovani F.; Gawroński M. P.; Peel M. W.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/261951
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