1. VLBI observations of bright AGN jets with KVN and VERA Array (KaVA): Evaluation of Imaging Capability
- Author
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Niinuma, Kotaro, Lee, Sang-Sung, Kino, Motoki, Sohn, Bong Won, Akiyama, Kazunori, Zhao, Guang-Yao, Sawada-Satoh, Satoko, Trippe, Sascha, Hada, Kazuhiro, Jung, Taehyun, Hagiwara, Yoshiaki, Dodson, Richard, Koyama, Shoko, Honma, Mareki, Nagai, Hiroshi, Chung, Aeree, Doi, Akihiro, Fujisawa, Kenta, Han, Myoung-Hee, Kim, Joeng-Sook, Lee, Jeewon, Lee, Jeong Ae, Miyazaki, Atsushi, Oyama, Tomoaki, Sorai, Kazuo, Wajima, Kiyoaki, Bae, Jaehan, Byun, Do-Young, Cho, Se-Hyung, Choi, Yoon Kyung, Chung, Hyunsoo, Chung, Moon-Hee, Han, Seog-Tae, Hirota, Tomoya, Hwang, Jung-Wook, Je, Do-Heung, Jike, Takaaki, Jung, Dong-Kyu, Jung, Jin-Seung, Kang, Ji-Hyun, Kang, Jiman, Kang, Yong-Woo, Kan-ya, Yukitoshi, Kanaguchi, Masahiro, Kawaguchi, Noriyuki, Kim, Bong Gyu, Kim, Hyo Ryoung, Kim, Hyun-Goo, Kim, Jaeheon, Kim, Jongsoo, Kim, Kee-Tae, Kim, Mikyoung, Kobayashi, Hideyuki, Kono, Yusuke, Kurayama, Tomoharu, Lee, Changhoon, Lee, Jung-Won, Lee, Sang Hyun, Minh, Young Chol, Matsumoto, Naoko, Nakagawa, Akiharu, Oh, Chung Sik, Oh, Se-Jin, Park, Sun-Youp, Roh, Duk-Gyoo, Sasao, Tetsuo, Shibata, Katsunori M., Song, Min-Gyu, Tamura, Yoshiaki, Wi, Seog-Oh, Yeom, Jae-Hwan, and Yun, Young Joo
- Subjects
Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
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 and 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 M 87. This is one of the initial result of KaVA early science. Our KaVA images reveal extended outflows with complex substructure such as knots and limb brightening, in agreement with previous Very Long Baseline Array (VLBA) observations. Angular resolutions are better than 1.4 and 0.8 milliarcsecond at 23 GHz and 43 GHz, respectively. KaVA achieves a high dynamic range of ~1000, more than three times the value achieved by VERA. We conclude that KaVA is a powerful array with a great potential for the study of AGN outflows, at least comparable to the best existing radio interferometric arrays., Comment: 15 pages, 10 figures, 6 tables, accepted for publication in PASJ
- Published
- 2014
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