Browse > Article
http://dx.doi.org/10.5303/JKAS.2022.55.6.207

RENOVATION OF SEOUL RADIO ASTRONOMY OBSERVATORY AND ITS FIRST MILLIMETER VLBI OBSERVATIONS  

Naeun, Shin (Department of Physics and Astronomy, Seoul National University)
Yong-Sun, Park (Department of Physics and Astronomy, Seoul National University)
Do-Young, Byun (Korea Astronomy and Space science Institute)
Jinguk, Seo (Department of Physics and Astronomy, Seoul National University)
Dongkok, Kim (Department of Physics and Astronomy, Seoul National University)
Cheulhong, Min (Department of Physics and Astronomy, Seoul National University)
Hyunwoo, Kang (Korea Astronomy and Space science Institute)
Keiichi, Asada (Academia Sinica Institute of Astronomy and Astrophysics)
Wen-Ping, Lo (Academia Sinica Institute of Astronomy and Astrophysics)
Sascha, Trippe (Department of Physics and Astronomy, Seoul National University)
Publication Information
Journal of The Korean Astronomical Society / v.55, no.6, 2022 , pp. 207-213 More about this Journal
Abstract
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.
Keywords
instrumentation: interferometers; techniques : high angular resolution;
Citations & Related Records
연도 인용수 순위
  • Reference
1 Algaba, J.-C., Zhao, G.-Y., Lee, S.-S., et al. 2015, Interferometric monitoring of Gamma-Ray bright Active Galactic Nuclei II: Frequency Phase Transfer, JKAS, 48, 237
2 Byun, D., & Yun, Y.-Z. 2002, Development of control softwares for the SRAO 6-meter telescope based on PCs running Linux, Exp. Astron., 14, 183   DOI
3 The Event Horizon Telescope Collaboration, Akiyama, K., Alberdi, A., Alef, W., et al. 2019, First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole, ApJL, 875, L1   DOI
4 Hudson, J. 1998, Ray-tracing the BIMA reflectors, BIMA Memoranda Series, No. 64
5 Hull, C., & Plambeck, R. 2015, The 1.3 mm full-stokes polarization system at CARMA, J. Astron. Instrum., 4, 1550005   DOI
6 Koo, B., Park, Y.-S., Hong, S., et al. 2003, Performance of the SRAO 6-meter radio telescope, JKAS, 36, 43
7 Lee, S.-S., Byun, D.-Y., Park, Y.-S., et al. 2003, Surface Adjustment of the SRAO 6-M Antenna Based on NearField Radio Holography at 86 GHz, International journal of infrared and millimeter waves, 24, 1687   DOI
8 Lee, J.-W., Kim, C.-H., Kang, H., et al. 2013, Development of 230 GHz radio receiver system for SRAO, JKAS, 46, 225
9 Oh, S.-J., Yeom, J.-H., Roh, D.-K., et al. 2017, A Study on the Test Results of 32 Gbps Observing System for Wideband VLBI Observation, Journal of the institute of signal processing and systems, 18, 13
10 Ogawa, M., Li, R., & Hashimoto, T. 1991, Thermal conductivities of magnetic intermetallic compounds for cryogenic regenerator, Cryogenics, 31, 405   DOI
11 Park, J., Kam, M., Trippe, S., et al. 2018, Revealing the Nature of Blazar Radio Cores through Multifrequency Polarization Observations with the Korean VLBI Network, ApJ, 860, 112   DOI
12 Plambeck, R., Thatte, N., & Sykes, P. 1992, A 4K Gifford-Mcmahon refrigerator for radio astronomy, 7th International cryocooler conference proceeding, 2, 401
13 Rioja, M. J., Dodson, R., Malarecki, J., et al. 2011, Exploration of Source Frequency Phase Referencing Techniques for Astrometry and Observations of Weak Sources with High Frequency Space Very Long Baseline Interferometry, AJ, 142, 157   DOI
14 Rioja, M. J., Dodson, R., Jung, T., et al. 2014, Verification of the Astrometric Performance of the Korean VLBI Network, Using Comparative SFPR Studies with the VLBA at 14/7 mm, AJ, 148, 84   DOI
15 Vertatschitsch, L., Primiani, R., Young, A., et al. 2015, R2DBE: A Wideband Digital Backend for the Event Horizon Telescope, PASP, 127, 1226   DOI
16 Wajima, K., Kino, M., & Kawakatu, N. 2020, Constraints on the Circumnuclear Disk through Free-Free Absorption in the Nucleus of 3C 84 with KaVA and KVN at 43 and 86 GHz, ApJ, 895, 35   DOI