Detection statistics of the RadioAstron AGN survey

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 con...

Full description

Saved in:
Bibliographic Details
Published in:Advances in space research Vol. 65; no. 2; pp. 705 - 711
Main Authors: Kovalev, Y.Y., Kardashev, N.S., Sokolovsky, K.V., Voitsik, P.A., An, T., Anderson, J.M., Andrianov, A.S., Avdeev, V.Yu, Bartel, N., Bignall, H.E., Burgin, M.S., Edwards, P.G., Ellingsen, S.P., Frey, S., García-Miró, C., Gawroński, M.P., Ghigo, F.D., Ghosh, T., Giovannini, G., Girin, I.A., Giroletti, M., Gurvits, L.I., Jauncey, D.L., Horiuchi, S., Ivanov, D.V., Kharinov, M.A., Koay, J.Y., Kostenko, V.I., Kovalenko, A.V., Kovalev, Yu.A., Kravchenko, E.V., Kunert-Bajraszewska, M., Kutkin, A.M., Likhachev, S.F., Lisakov, M.M., Litovchenko, I.D., McCallum, J.N., Melis, A., Melnikov, A.E., Migoni, C., Nair, D.G., Pashchenko, I.N., Phillips, C.J., Polatidis, A., Pushkarev, A.B., Quick, J.F.H., Rakhimov, I.A., Reynolds, C., Rizzo, J.R., Rudnitskiy, A.G., Savolainen, T., Shakhvorostova, N.N., Shatskaya, M.V., Shen, Z.-Q., Shchurov, M.A., Vermeulen, R.C., de Vicente, P., Wolak, P., Zensus, J.A., Zuga, V.A.
Format: Journal Article
Language:English
Published: Elsevier Ltd 15-01-2020
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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.
ISSN:0273-1177
1879-1948
DOI:10.1016/j.asr.2019.08.035