activity
20142026
most citedVLBI observations of bright AGN jets with KVN and VERA Array (KaVA): Evaluation of Imaging Capability

44 citations · 131 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2022★ 7 cited

The Astrometric Animation of Water Masers towards the Mira Variable BX Cam

Shuangjing Xu, Hiroshi Imai, Youngjoo Yun +20

We report VLBI monitoring observations of the 22 GHz water (HO) masers around the Mira variable BX Cam, which were carried out as a part of the EAVN Synthesis of Stellar Mase…

astro-ph.SR2020★ 11 cited

Asymmetric distributions of H2O and SiO masers towards V627 Cas

Haneul Yang, Se-Hyung Cho, Youngjoo Yun +7

We performed simultaneous observations of the H2O 6(1,6) - 5(2,3) (22.235080 GHz) and SiO v= 1, 2, J = 1 - 0, SiO v = 1, J = 2 - 1, 3 - 2 (43.122080, 42.820587, 86.243442, and 129.…

astro-ph.SR2018★ 12 cited

Simultaneous VLBI Astrometry of H2O and SiO Masers toward the Semiregular Variable R Crateris

Dong-Jin Kim, Se-Hyung Cho, Youngjoo Yun +7

We obtained, for the first time, astrometrically registered maps of the 22.2 GHz H2O and 42.8, 43.1, and 86.2 GHz SiO maser emission toward the semiregular b-type variable (SRb) R…

astro-ph.SR2018★ 24 cited

Astrometrically registered maps of H2O and SiO masers toward VX Sagittarii

Dong-Hwan Yoon, Se-Hyung Cho, Youngjoo Yun +8

The supergiant VX Sagittarii is a strong emitter of both H2O and SiO masers. However, previous VLBI observations have been performed separately, which makes it difficult to spatial…

astro-ph.SR2015★ 2 cited

KVN Monitoring Obsevations toward the Recent Outburst Symbiotic Star V407 Cygni

Se-Hyung Cho, Jaeheon Kim, Youngjoo Yun

Simultaneous time monitoring observations of HO and SiO maser lines were performed toward the D-type symbiotic binary system V407 Cyg with the Korean VLBI Network single dish…

astro-ph.SR2014★ 3 cited

First detection of 22 GHz H2O masers in TX Camelopardalis

Se-Hyung Cho, Jaeheon Kim, Youngjoo Yun

Simultaneous time monitoring observations of HO , SiO = 1--0, 2--1, 3--2, and SiO = 0, = 1--0 lines were carried out in the direction of the…