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East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA plus Tianma plus Nanshan | |
Cui, Yu-Zhu1,2; Hada, Kazuhiro1,2; Kino, Motoki2,3; Sohn, Bong-Won4,5,6; Park, Jongho7; Ro, Hyun-Wook4,5; Sawada-Satoh, Satoko8; Jiang, Wu9,11; Cui, Lang10,11![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | |
2021-10-01 | |
Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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ISSN | 1674-4527 |
Volume | 21Issue:8Pages:205 |
Contribution Rank | 4 |
Abstract | The East Asian Very Long Baseline Interferometry (VLBI) Network (EAVN) is a rapidly evolving international VLBI array that is currently promoted under joint efforts among China, Japan and Korea. EAVN aims at forming a joint VLBI Network by combining a large number of radio telescopes distributed over East Asian regions. After the combination of the Korean VLBI Network (KVN) and the VLBI Exploration of Radio Astrometry (VERA) into KaVA, further expansion with the joint array in East Asia is actively promoted. Here we report the first imaging results (at 22 and 43 GHz) of bright radio sources obtained with KaVA connected to Tianma 65-m and Nanshan 26-m Radio Telescopes in China. To test the EAVN imaging performance for different sources, we observed four active galactic nuclei (AGN) having different brightness and morphology. As a result, we confirmed that the Tianma 65-m Radio Telescope (TMRT) significantly enhances the overall array sensitivity, a factor of 4 improvement in baseline sensitivity and 2 in image dynamic range compared to the case of KaVA only. The addition of the Nanshan 26-m Radio Telescope (NSRT) further doubled the east-west angular resolution. With the resulting high-dynamic-range, high-resolution images with EAVN (KaVA+TMRT+NSRT), various fine-scale structures in our targets, such as the counter-jet in M87, a kink-like morphology of the 3C 273 jet and the weak emission in other sources are successfully detected. This demonstrates the powerful capability of EAVN to study AGN jets and to achieve other science goals in general. Ongoing expansion of EAVN will further enhance the angular resolution, detection sensitivity and frequency coverage of the network. |
Keyword | galaxies active galaxies jets instrumentation interferometers radio continuum galaxies |
DOI | 10.1088/1674-4527/21/8/205 |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | RADIO JET ; AGN JETS ; TELESCOPE ; GALAXIES |
Funding Project | Graduate University for Advanced Studies (SOKENDAI) ; Japanese Government (MEXT) Scholarship ; JSPS KAKENHI[JP18K03656] ; JSPS KAKENHI[JP18H03721] ; JSPS KAKENHI[JP19H01943] ; JSPS KAKENHI[JP18KK0090] ; Mitsubishi Foundation[201911019] ; EACOA Fellowship - East Asia Core Observatories Association of the Academia Sinica Institute of Astronomy and Astrophysics ; EACOA Fellowship - East Asia Core Observatories Association of the National Astronomical Observatory of Japan ; EACOA Fellowship - East Asia Core Observatories Association of the Center for Astronomical Mega-Science ; EACOA Fellowship - East Asia Core Observatories Association of the Chinese Academy of Sciences ; EACOA Fellowship - East Asia Core Observatories Association of the Korea Astronomy and Space Science Institute ; National Research Foundation (NRF) of Korea[2014H1A2A1018695] ; National Research Foundation (NRF) of Korea[2015H1A2A1033752] ; NRF[2019R1F1A1059721] ; Major Program of the National Natural Science Foundation of China (NSFC)[11590780] ; Major Program of the National Natural Science Foundation of China (NSFC)[11590784] ; Knowledge Innovation Program of the Chinese Academy of Sciences[KJCX1-YW-18] ; Scientific Program of Shanghai Municipality[08DZ1160100] ; Key Laboratory for Radio Astronomy, CAS ; NSFC[11803071] ; NSFC[U2031212] ; NSFC[61931002] ; NSFC[11933007] ; National Key R&D Program of China[2018YFA0404602] ; CAS 'Light of West China' Program[2018-XBQNXZ-B-021] ; Youth Innovation Promotion Association of the CAS[2017084] ; Fundamental Research Grant Scheme (FRGS)[FRGS/1/2019/STG02/UM/02/6] ; Max Planck Partner Group of the MPG ; CAS ; Research Program of Fundamental and Frontier Sciences, CAS[ZDBS-LY-SLH011] |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000711660200001 |
Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
Funding Organization | Graduate University for Advanced Studies (SOKENDAI) ; Japanese Government (MEXT) Scholarship ; JSPS KAKENHI ; Mitsubishi Foundation ; EACOA Fellowship - East Asia Core Observatories Association of the Academia Sinica Institute of Astronomy and Astrophysics ; EACOA Fellowship - East Asia Core Observatories Association of the National Astronomical Observatory of Japan ; EACOA Fellowship - East Asia Core Observatories Association of the Center for Astronomical Mega-Science ; EACOA Fellowship - East Asia Core Observatories Association of the Chinese Academy of Sciences ; EACOA Fellowship - East Asia Core Observatories Association of the Korea Astronomy and Space Science Institute ; National Research Foundation (NRF) of Korea ; NRF ; Major Program of the National Natural Science Foundation of China (NSFC) ; Knowledge Innovation Program of the Chinese Academy of Sciences ; Scientific Program of Shanghai Municipality ; Key Laboratory for Radio Astronomy, CAS ; NSFC ; National Key R&D Program of China ; CAS 'Light of West China' Program ; Youth Innovation Promotion Association of the CAS ; Fundamental Research Grant Scheme (FRGS) ; Max Planck Partner Group of the MPG ; CAS ; Research Program of Fundamental and Frontier Sciences, CAS |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/4366 |
Collection | 射电天文研究室_星系宇宙学研究团组 射电天文研究室_脉冲星研究团组 射电天文研究室_26米望远镜运行组 射电天文研究室_微波技术实验室 射电天文研究室_行星科学研究团组 射电天文研究室_南山观测站 科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章 |
Corresponding Author | Cui, Yu-Zhu |
Affiliation | 1.Grad Univ Adv Studies, Dept Astron Sci, SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 2.Natl Astron Observ Japan, Mizusawa VLBI Observ, 2-12 Hoshigaoka, Oshu, Iwate 0230861, Japan 3.Kogakuin Univ Technol & Engn, Acad Support Ctr, 2665-1 Nakano, Hachioji, Tokyo 1920015, Japan 4.Korea Astron & Space Sci Inst, Daejeon 34055, South Korea 5.Yonsei Univ, Dept Astron, 50 Yonsei Ro, Seoul 03722, South Korea 6.Univ Sci & Technol, Dept Astron & Space Sci, 217 Gajeong Ro, Daejeon, South Korea 7.Acad Sinica, Inst Astron & Astrophys, 645 N Aohoku Pl, Hilo, HI 96720 USA 8.Yamaguchi Univ, Grad Sch Sci & Technol Innovat, Yoshida 1677-1, Yamaguchi, Yamaguchi 7538512, Japan 9.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China 10.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 11.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 12.Univ Tokyo, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan 13.CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, E-18008 Granada, Spain 14.Univ Malaya, Fac Sci, Dept Phys, Kuala Lumpur 50603, Malaysia 15.Ibaraki Univ, Ctr Astron, 2-1-1 Bunkyo, Mito, Ibaraki 3108512, Japan 16.Space Light Lab, 77,Yangjaedae Ro 86 Rd, Seoul, South Korea 17.MIT, Haystack Observ, 99 Millstone Rd, Westford, MA 01886 USA 18.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA 19.Toyo Univ, Bunkyo Ku, 5-28-20 Hakusan, Tokyo 1128606, Japan 20.Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea 21.Max Planck Inst Radio Astron, Hugel 69, D-53121 Bonn, Germany 22.Seoul Natl Univ, SNU Astron Res Ctr, Seoul 08826, South Korea |
Recommended Citation GB/T 7714 | Cui, Yu-Zhu,Hada, Kazuhiro,Kino, Motoki,et al. East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA plus Tianma plus Nanshan[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2021,21(8):205. |
APA | Cui, Yu-Zhu.,Hada, Kazuhiro.,Kino, Motoki.,Sohn, Bong-Won.,Park, Jongho.,...&Zhang, Bo.(2021).East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA plus Tianma plus Nanshan.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,21(8),205. |
MLA | Cui, Yu-Zhu,et al."East Asian VLBI Network observations of active galactic nuclei jets: imaging with KaVA plus Tianma plus Nanshan".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 21.8(2021):205. |
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