Renovation of Seoul Radio Astronomy Observatory and Its First Millimeter VLBI Observations

• Published in: arXiv.org
• Main Authors: Shin, Naeun, Yong-Sun, Park, Do-Young, Byun, Seo, Jinguk, Kim, Dongkok, Cheulhong Min, Kang, Hyunwoo, Asada, Keiichi, Wen-Ping Lo, Trippe, Sascha
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 27.01.2023
• Subjects: Event horizon; Extremely high frequencies; Millimeter waves; Observatories; Physics - Instrumentation and Methods for Astrophysics; Radio astronomy; Radio telescopes; Receivers & amplifiers; Very long base interferometry
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2301.11566

The Seoul Radio Astronomy Observatory (SRAO) operates a 6.1-meter radio telescope on the Gwanak campus of Seoul National University. We present the efforts to reform SRAO to a Very Long Baseline Interferometry (VLBI) station, motivated by recent achievements by millimeter interferometer networks such as Event Horizon Telescope, East Asia VLBI Network, and Korean VLBI Network (KVN). For this goal, we installed a receiver that had been used in the Combined Array for Research in Millimeter-wave Astronomy and a digital backend, including an H-maser clock. The existing hardware and software were also revised, which had been dedicated only to single-dish operations. After several years of preparations and test observations in 1 and 3-millimeter bands, a fringe was successfully detected toward 3C 84 in 86 GHz in June 2022 for a baseline between SRAO and KVN Ulsan station separated by 300 km. Thanks to the dual frequency operation of the receiver, the VLBI observations will soon be extended to the 1 mm band and verify the frequency phase referencing technique between 1 and 3-millimeter bands.