activity
20182026
most citedRevealing the Nature of Blazar Radio Cores through Multi-Frequency Polarization Observations with the Korean VLBI Network

28 citations · 83 across the 11 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

The 2015-2017 Large EVPA Rotation in OJ 287: Dominant Propagating Component in a Helical Magnetic Field with Time-Dependent Viewing Geometry

Wanchaloem Khwammai, Minchul Kam, Motoki Kino +11

We present high-cadence, multi-frequency monitoring of the blazar OJ 287 using KVN (22--129 GHz), ALMA (91.5--343.5 GHz), and Metsähovi (37 GHz), covering 2012--2023, together with…

astro-ph.IM2026

Verification of the Polarimetric Capability of the East Asia VLBI Network

Yunjeong Lee, Jongho Park, Do-Young Byun +10

The East Asia VLBI Network (EAVN) has recently enabled dual-polarization observations at and . We present the first systematic verification of its polarimetr…

astro-ph.GA2026

A Unified Origin of Faraday Rotation toward 3C 84: The Circumnuclear Ambient Medium within the Parsec-Scale Bondi Radius of the Host Galaxy NGC 1275

Minchul Kam, Jongho Park, Sascha Trippe +11

We present multi-frequency polarimetric observations of 3C 84 obtained with the Korean VLBI Network at 43-141 GHz, the Very Long Baseline Array at 43 GHz, and the High Sensitivity…

astro-ph.HE2025

Helical Magnetic Field in the Acceleration--Collimation Zone of the M87 Jet

Jongho Park, Kazuya Takahashi, Kenji Toma +10

Relativistic jets from supermassive black holes are expected to be magnetically launched and guided, with magnetic energy systematically converted to bulk kinetic energy throughout…

astro-ph.GA2025

Monitoring of 3C 286 with ALMA, IRAM, and SMA from 2006 to 2025: Stability, Synchrotron Ages, and Frequency-Dependent Polarization Attributed to Core-Shift

Minchul Kam, Hiroshi Nagai, Motoki Kino +23

We present the results of multi-frequency monitoring of the radio quasar 3C 286, conducted using three instruments: ALMA at 91.5, 103.5, 233.0, and 343.4 GHz, the IRAM 30-m Telesco…

astro-ph.GA2025

Polarization flare of 3C 454.3 in millimeter wavelengths seen from decadal polarimetric observations

Hyeon-Woo Jeong, Sang-Sung Lee, Sincheol Kang +6

This study investigates polarimetric characteristics of the blazar 3C~454.3 at 22-129~GHz using decadal~(2011-2022) data sets. In addition, we also delve into the origin of the pol…

astro-ph.HE2024★ 17 cited

Discovery of Limb Brightening in the Parsec-scale Jet of NGC 315 through Global Very Long Baseline Interferometry Observations and Its Implications for Jet Models

Jongho Park, Guang-Yao Zhao, Masanori Nakamura +19

We report the first observation of the nearby giant radio galaxy NGC 315 using a global VLBI array consisting of 22 radio antennas located across five continents, including high-se…

astro-ph.HE2023★ 13 cited

Observational Evidence to Support a Dense Ambient Medium Shaping the Jet in 3C 84

Jongho Park, Motoki Kino, Hiroshi Nagai +4

Highly collimated relativistic jets are a defining feature of certain active galactic nuclei (AGN), yet their formation mechanism remains elusive. Previous observations and theoret…

astro-ph.HE2023★ 1 cited

Evolution of the Termination Region of the Parsec-Scale Jet of 3C 84 Over the Past 20 Years

Minchul Kam, Jeffrey A. Hodgson, Jongho Park +4

We present the kinematics of the parsec-scale jet in 3C 84 from 2003 November to 2022 June observed with the Very Long Baseline Array (VLBA) at 43 GHz. We find that the C3 componen…

astro-ph.HE2023★ 6 cited

Probing the Heart of Active Narrow-line Seyfert 1 Galaxies with VERA Wideband Polarimetry

Mieko Takamura, Kazuhiro Hada, Mareki Honma +9

We explored the parsec-scale nuclear regions of a sample of radio-loud narrow-line Seyfert 1 galaxies (NLSy1s) using the VLBI Exploration of Radio Astronomy (VERA) wideband (at a r…

astro-ph.GA2022

Using the Crab Nebula as Polarization Angle Calibrator for the Korean VLBI Network

Minchul Kam, Sascha Trippe, Do-Young Byun +5

The Crab nebula is widely used as a polarization angle calibrator for single-dish radio observations because of its brightness, high degree of linear polarization, and well-known p…

astro-ph.GA2021★ 18 cited

A persistent double nuclear structure in 3C 84

Junghwan Oh, Jeffrey A. Hodgson, Sascha Trippe +11

3C 84 (NGC 1275) is the radio source at the center of the Perseus Cluster and exhibits a bright radio jet. We observed the source with the Global Millimeter VLBI Array (GMVA) betwe…

astro-ph.HE2018★ 28 cited

Revealing the Nature of Blazar Radio Cores through Multi-Frequency Polarization Observations with the Korean VLBI Network

Jongho Park, Minchul Kam, Sascha Trippe +13

We study the linear polarization of the radio cores of eight blazars simultaneously at 22, 43, and 86 GHz with observations obtained by the Korean VLBI Network (KVN) in three epoch…