Volume 330, Issue 2-3 pp. 128-132
Original Paper

Long-term radio behaviour of GPS sources and candidates

M. TornikoskiI. Torniainen

I. Torniainen

Metsähovi Radio Observatory, Helsinki University of Technology TKK, Metsähovintie 114, 02540 Kylmälä, Finland

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A. Lähteenmäki

A. Lähteenmäki

Metsähovi Radio Observatory, Helsinki University of Technology TKK, Metsähovintie 114, 02540 Kylmälä, Finland

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T. Hovatta

T. Hovatta

Metsähovi Radio Observatory, Helsinki University of Technology TKK, Metsähovintie 114, 02540 Kylmälä, Finland

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E. Nieppola

E. Nieppola

Metsähovi Radio Observatory, Helsinki University of Technology TKK, Metsähovintie 114, 02540 Kylmälä, Finland

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M. Turunen

M. Turunen

Metsähovi Radio Observatory, Helsinki University of Technology TKK, Metsähovintie 114, 02540 Kylmälä, Finland

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M. Lainela

M. Lainela

Tuorla Observatory, University of Turku, Väisälantie 20, 21500 Piikkiö, Finland

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E. Valtaoja

E. Valtaoja

Tuorla Observatory, University of Turku, Väisälantie 20, 21500 Piikkiö, Finland

Department of Physics, University of Turku, 20100 Turku, Finland

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M.F. Aller

M.F. Aller

Department of Astronomy, University of Michigan, Ami Arbor, MI, 48190, USA

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H.D. Aller

H.D. Aller

Department of Astronomy, University of Michigan, Ami Arbor, MI, 48190, USA

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M. Mingaliev

M. Mingaliev

Special Astrophysics Observatory, RAS, Nizhnij Arkhyz, Karachaevo-Cherkesia, 369167 Russia

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S. Trushkin

S. Trushkin

Special Astrophysics Observatory, RAS, Nizhnij Arkhyz, Karachaevo-Cherkesia, 369167 Russia

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First published: 13 February 2009
Citations: 14

Abstract

This paper is a summary of the work that our group has done (and recently published in several papers) on long-term radio variability of GPS sources. We have studied the long-term (up to 30 years) variability of GPS sources and candidates, with emphasis on the high-frequency radio domain. Our data sets show that only a relatively small number of these sources retain their convex spectra when they are monitored densely and for long periods of time. The current GPS samples are especially contaminated by small, beamed blazar-type sources. Also the remaining population with consistently convex GPS-type spectra seems to be heterogeneous, falling into several subpopulations when their observed properties are used for clustering them through a self-organizing map (© 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

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