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Detection statistics of the RadioAstron AGN survey

journal contribution
posted on 2023-05-20, 16:28 authored by Kovalev, YY, Kardashev, NS, Sokolovsky, KV, Voitsik, PA, An, T, Anderson, JM, Andrianov, AS, Avdeev, VY, Bartel, N, Bignall, HE, Burgin, MS, Edwards, PG, Simon EllingsenSimon Ellingsen, Frey, S, Garcia-Miro, C, Gawronski, MP, Ghigo, FD, Ghosh, T, Giovannini, G, Girin, IA, Giroletti, M, Gurvits, LI, Jauncey, DL, Horiuchi, S, Ivanov, DV, Kharinov, MA, Koay, JY, Kostenko, VI, Kovalenko, AV, Kovalev, YA, Kravchenko, EV, Kunert-Bajraszewska, M, Kutkin, AM, Likhachev, SF, Lisakov, MM, Litovchenko, ID, Jamie McCallumJamie McCallum, Melis, A, Melnikov, AE, Migoni, C, Nair, DG, Pashchenko, IN, Phillips, CJ, Polatidis, A, Pushkarev, AB, Quick, JFH, Rakhimov, IA, Reynolds, C, Rizzo, JR, Rudnitskiy, AG, Savolainen, T, Shakhvorostova, NN, Shatskaya, MV, Shen, Z-Q, Shchurov, MA, Vermeulen, RC, de Vicente, P, Wolak, P, Zensus, JA, Zuga, VA
The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightness of AGN cores in order to better understand the physics of their emission while taking interstellar scattering into consideration. In this paper we present detection statistics for observations on ground-space baselines of a complete sample of radio-strong AGN at the wavelengths of 18, 6, and 1.3 cm. Two-thirds of them are indeed detected by RadioAstron and are found to contain extremely compact, tens to hundreds of μas structures within their cores.

History

Publication title

Advances in Space Research

Volume

65

Pagination

705-711

ISSN

0273-1177

Department/School

School of Natural Sciences

Publisher

Pergamon-Elsevier Science Ltd

Place of publication

The Boulevard, Langford Lane, Kidlington, Oxford, England, Ox5 1Gb

Rights statement

Copyright 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.

Repository Status

  • Restricted

Socio-economic Objectives

Expanding knowledge in the physical sciences

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