Volume 330, Issue 2-3 pp. 223-225
Original Paper

High Frequency Peakers: The faint sample

C. StanghelliniD. Dallacasa

D. Dallacasa

Istituto di Radioastronomia – INAF, Via P. Gobetti 101, I-40129 Bologna, Italy

Dipartimento di Astronomia – Università di Bologna, Via Ranzani 1, I-40127 Bologna, Italy

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M. Orienti

M. Orienti

Istituto di Radioastronomia – INAF, Via P. Gobetti 101, I-40129 Bologna, Italy

Instituto de Astrofísica de Canarias, C/ Via Láctea s/n, E-38200 La Laguna, Tenerife, Spain

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First published: 13 February 2009
Citations: 14

Abstract

We present a sample of sources with convex radio spectra peaking at frequencies above a few GHz, known as “High Frequency Peakers” (HFPs). A “bright” sample with a flux density limit of 300 mJy at 5 GHz has been presented by Dallacasa et al. (2000). Here we present the “faint” sample with flux density between 50 and 300 mJy at 5 GHz, restricted to the area around the North Galactic Cap, where the FIRST catalogue is available. The candidates have been observed with the VLA at several frequencies ranging from 1.4 to 22 GHz, in order to derive a simultaneous radio spectrum. The final list of confirmed HFP sources consists of 61 objects (© 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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