Skip to main navigation Skip to search Skip to main content

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

  • Kotaro Niinuma*
  • , Sang-Sung Lee
  • , Motoki Kino
  • , Bong Won Sohn
  • , Kazunori Akiyama
  • , Guang-Yao Zhao
  • , Satoko Sawada-Satoh
  • , Sascha Trippe
  • , Kazuhiro Hada
  • , Taehyun Jung
  • , Yoshiaki Hagiwara
  • , Richard Dodson
  • , Shoko Koyama
  • , Mareki Honma
  • , Hiroshi Nagai
  • , Aeree Chung
  • , Akihiro Doi
  • , Kenta Fujisawa
  • , Myoung-Hee Han
  • , Joeng-Sook Kim
  • Jeewon Lee, Jeong Ae Lee, Atsushi Miyazaki, Tomoaki Oyama, Kazuo Sorai, Kiyoaki Wajima, Jaehan Bae, Do-Young Byun, Se-Hyung Cho, Yoon Kyung Choi, Hyunsoo Chung, Moon-Hee Chung, Seog-Tae Han, Tomoya Hirota, Jung-Wook Hwang, Do-Heung Je, Takaaki Jike, Dong-Kyu Jung, Jin-Seung Jung, Ji-Hyun Kang, Jiman Kang, Yong-Woo Kang, Yukitoshi Kan-Ya, Masahiro Kanaguchi, Noriyuki Kawaguchi, Bong Gyu Kim, Hyo Ryoung Kim, Hyun-Goo Kim, Jaeheon Kim, Jongsoo Kim
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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 (23-43GHz bands) observations in East Asia. Here, we report the first imaging observations of three bright active galactic nuclei (AGNs) known for their complex morphologies: 4C39.25, 3C273, and M87. This is one of the initial results of KaVA's early operation. Our KaVA images reveal extended outflows with complex substructures 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 mas at 23 and 43GHz, 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.

Original languageEnglish
Article number103
JournalPublications of the Astronomical Society of Japan
Volume66
Issue number6
DOIs
Publication statusPublished - Dec 2014

Keywords

  • Galaxies: active
  • Galaxies: jets
  • Radio continuum: galaxies
  • Techniques: interferometric

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'VLBI observations of bright AGN jets with the KVN and VERA Array (KaVA): Evaluation of imaging capability'. Together they form a unique fingerprint.

Cite this