| Issue |
A&A
Volume 692, December 2024
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/202452745e | |
| Published online | 02 December 2024 | |
Unveiling the bent-jet structure and polarization of OJ 287 at 1.7 GHz with space VLBI (Corrigendum)
1
Instituto de Astrofísica de Andalucía-CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, Spain
2
Korea Astronomy and Space Science Institute, Daedeok-daero 776, Yuseong-gu, Daejeon 34055, Republic of Korea
3
Department of Astronomy, Yonsei University, Yonsei-ro 50, Seodaemun-gu, 03722 Seoul, Republic of Korea
4
INAF – Istituto di Radioastronomia, Via P. Gobetti 101, I-40129 Bologna, Italy
5
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
6
Lebedev Physical Institute of the Russian Academy of Sciences, Leninsky Prospekt 53, 119991 Moscow, Russia
7
Moscow Institute of Physics and Technology, Institutsky Per. 9, Dolgoprudny, Moscow Region 141700, Russia
8
Crimean Astrophysical Observatory, 98409 Nauchny, Crimea
9
Joint Institute for VLBI ERIC (JIVE), Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands
10
Faculty of Aerospace Engineering, Delft University of Technology, Kluyverweg 1, 2629 HS Delft, The Netherlands
11
Department of Astronomy and Atmospheric Sciences, Kyungpook National University, Daegu 702-701, Republic of Korea
12
Institut de Radioastronomie Millimétrique, Avenida Divina Pastora, 7, Local 20, E18012 Granada, Spain
13
Institute of Astrophysics, Foundation for Research and Technology – Hellas, N. Plastira 100, Voutes, GR-70013 Heraklion, Greece
⋆ Corresponding author; icho@kasi.re.kr
Key words: galaxies: active / galaxies: jets / quasars: supermassive black holes / radio continuum: galaxies / errata / addenda
The expression “suggesting a model” was not an accurate description of a point made in Komossa et al. (2023), which presented an alternative supermassive black hole binary “measurement” supporting a model that involves a primary supermassive black hole of a much lower mass. Additionally, there was misinformation regarding the programs that provided single-dish polarization data from Effelsberg. The previous program, F-GAMMA/QUIVER, was terminated in January 2015, and a new program, MOMO (Komossa et al. 2015, 2023), was launched in December 2015. Therefore, the name of the program referenced in the paper that utilized data from April 7, 2016, should be corrected to MOMO, not F-GAMMA/QUIVER.
References
- Komossa, S., Myserlis, I., Angelakis, E., et al. 2015, ATel, 8411, 1 [NASA ADS] [Google Scholar]
- Komossa, S., Grupe, D., Kraus, A., et al. 2023, MNRAS, 522, L84 [NASA ADS] [CrossRef] [Google Scholar]
© The Authors 2024
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