activity
20142017
most citedInterferometric Monitoring of Gamma-ray Bright AGNs I: Results of Single-epoch Multifrequency Observations

33 citations · 166 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA201715 cited

Korean VLBI Network Calibrator Survey (KVNCS): 1. Source Catalog Of KVN Single Dish Flux Density Measurement In The K And Q Bands

Jeong Ae Lee, Bong Won Sohn, Taehyun Jung +2

We present the catalog of the KVN Calibrator Survey (KVNCS). This first part of the KVNCS is a single dish radio survey conducted at 22 (K band) and 43 GHz (Q band) simultaneously…

astro-ph.GA201719 cited

Linear Polarization of Class I Methanol Masers in Massive Star-Forming Regions

Ji-hyun Kang, Do-Young Byun, Kee-Tae Kim +3

Class I methanol masers are found to be good tracers of the interaction between outflows from massive young stellar objects with their surrounding media. Although polarization obse…

astro-ph.GA201633 cited

Interferometric Monitoring of Gamma-ray Bright AGNs I: Results of Single-epoch Multifrequency Observations

Sang-Sung Lee, Kyoaki Wajima, Juan-Carlos Algaba +12

We present results of single-epoch very long baseline interferometry (VLBI) observations of gamma-ray bright active galactic nuclei (AGNs) using the Korean VLBI Network (KVN) at 22…

astro-ph.GA201614 cited

Spatially Resolved HCN Absorption Features in the Circumnuclear Region of NGC 1052

Satoko Sawada-Satoh, Duk-Gyoo Roh, Se-Jin Oh +7

We present the first VLBI detection of HCN molecular absorption in the nearby active galactic nucleus NGC 1052. Utilizing the 1 milliarcsecond resolution achieved by the Korean VLB…

astro-ph.HE201622 cited

Probing the gamma-ray variability in 3C279 using broadband observations

B. Rani, T. P. Krichbaum, S. -S. Lee +5

We present the results of a broadband radio-to-GeV observing campaign organized to get a better understanding of the radiation processes responsible for the -ray flares observed…

astro-ph.IM201428 cited

Astrometrically Registered Simultaneous Observations of the 22 GHz HO and the 43GHz SiO masers towards R Leonis Minoris using KVN and Source/Frequency Phase Referencing

Richard Dodson, María J. Rioja, Tae-Hyun Jung +22

Oxygen-rich Asymptotic Giant Branch (AGB) stars can be intense emitters of SiO (=1 and 2, J=10) and HO maser lines at 43 and 22 GHz, respectively. VLBI observat…