VLBI observations of bright AGN jets with the KVN and VERA Array (KaVA): Evaluation of imaging capability

@inproceedings{Niinuma2014VLBIOO,
  title={VLBI observations of bright AGN jets with the KVN and VERA Array (KaVA): Evaluation of imaging capability},
  author={Kotaro Niinuma and Sang-Sung Lee and Motoki Kino and Bong Won Sohn and Kazunori Akiyama and Guang-yao Zhao and Satoko Sawada-Satoh and Sascha Trippe and Kazuhiro Hada and Taehyun Jung and Yoshiaki Hagiwara and Richard Dodson and Shoko Koyama and Mareki Honma and Hiroshi Nagai and Aeree Chung and Akihiro Doi and Kenta Fujisawa and Myoung-Hee Han and Joeng-Sook Kim and Jee Won Lee and Jeong Ae Lee and Atsushi Miyazaki and Tomoaki Oyama and Kazuo Sorai and Kiyoaki Wajima and Joonwoo Bae and D. -J. Byun and Sehyung Cho and Yoon Kyung Choi and Hyunsoo Chung and Moon-Hee Chung and Seog-Tae Han and Takeshi Hirota and Jung-Wook Hwang and Do-Heung Je and Takaaki Jike and Dong-Kyu Jung and Jin-Seung Jung and Ji-Hyun Kang and Jiman Kang and Y. Kang and Yukitoshi Kan-ya and Masahiro Kanaguchi and Noriyuki Kawaguchi and Bong Gyu Kim and Hyo Ryoung Kim and Hyun-Goo Kim and Jaeheon Kim and Jongsoo Kim and Kee-Tae Kim and Mikyoung Kim and Hisayuki Kobayashi and Y. Kono and Tomoharu Kurayama and Chang Hoon Lee and Jung-Won Lee and Sang hyun Lee and Young Chol Minh and Naomichi Matsumoto and Akiharu Nakagawa and Chung Sik Oh and Se-jin Oh and Sun-Youp Park and Duk-Gyoo Roh and Tetsuo Sasao and Katsunori M. I. Shibata and Min-Gyu Song and Yoshiaki Tamura and Seog-Oh Wi and Jae-Hwan Yeom and Young joo Yun},
  year={2014}
}
The Korean very-long-baseline interferometry (VLBI) network (KVN) and VLBI Exploration of Radio Astrometry (VERA) Array (KaVA) is the first international VLBI array dedicated to high-frequency (23-43 GHz bands) observations in East Asia. Here, we report the first imaging observations of three bright active galactic nuclei (AGNs) known for their complex morphologies: 4C 39.25, 3C 273, and M87. This is one of the initial results of KaVA's early operation. Our KaVA images reveal extended outflows… CONTINUE READING

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