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Astrometric Apparent Motion of High-redshift Radio Sources

  • Authors: Oleg Titov, Sándor Frey, Alexey Melnikov, Fengchun Shu, Bo Xia, Javier González, Belén Tercero, Leonid Gurvits, Aletha de Witt, Jamie McCallum, Mikhail Kharinov, Vladimir Zimovsky, Máté Krezinger

Oleg Titov et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 8.

Evolution of the position of the source 2101+600 in the sky plane over the period from 2017.0 to 2021.2. The R.A. and decl. time series (Figure 7) were fitted by the linear trend and harmonic signal with the period of 3 yr. This approximation is shown by the black curve. The estimates of the amplitude of variations are 0.28 ± 0.05 mas in R.A. and 0.11 ± 0.05 mas in decl.. The reference point corresponds to the solution aus2020a. crf. The error bars are from Figure 7, but referred to the fitting curve here.

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