Astrometric Apparent Motion of High-redshift Radio Sources
Radio-loud quasars at high redshift (z ≥ 4) are rare objects in the universe and rarely observed with Very Long Baseline Interferometry (VLBI). But some of them have flux density sufficiently high for monitoring of their apparent position. The instability of the astrometric positions could be linked to the astrophysical process in the jetted active galactic nuclei in the early universe. Regular observations of the high-redshift quasars are used for estimating their apparent proper motion over several years. We have undertaken regular VLBI observations of several high-redshift quasars at 2.3 GHz (S band) and 8.4 GHz (X band) with a network of five radio telescopes: 40 m Yebes (Spain), 25 m Sheshan (China), and three 32 m telescopes of the Quasar VLBI Network (Russia)—Svetloe, Zelenchukskaya, and Badary. Additional facilities joined this network occasionally. The sources have also been observed in three sessions with the European VLBI Network in 2018–2019 and one Long Baseline Array experiment in 2018. In addition, several experiments conducted with the Very Long Baseline Array in 2017–2018 were used to improve the time sampling and the statistics. Based on these 37 astrometric VLBI experiments between 2017 and 2021, we estimated the apparent proper motions of four quasars: 0901+697, 1428+422, 1508+572, and 2101+600.
Citation: Oleg Titov <i>et al </i>2023 <i>AJ</i><b> 165</b> 69
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Role Organisation / Individual Name Details Author Titov, O.
Internal Contact Author Frey, S.
External Contact Author Melnikov, A.
External Contact Author Shu, F.
External Contact Author Xia, B.
External Contact Author Gonzalez, J.
External Contact Author Tercero, B.
External Contact Author Gurvits, L.
External Contact Author de Witt, A.
External Contact Author McCallum, J.
External Contact Author Kharinov, M.
External Contact Author Zimovsky, V.
External Contact Author Krezinger, M.
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Volume 165 Number 2
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Very Long Baseline Interferometry - VLBI
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geodesy
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International Celestial Reference System - ICRF
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Radiometrics
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AU/NZS ISO 19115-1:2014
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