activity
20242026
collaborators

13 papers

astro-ph.HE2026

A Universal Physics Defining the Radiation Spectra of Blazars and Gamma-Ray Bursts

Z. Lucas Uhm, Sang-Sung Lee, Bing Zhang +5

Blazars and gamma-ray bursts (GRBs) are both cosmic beacons of extreme energy release powered by relativistic jets. However, they originate from tremendously different environments…

astro-ph.GA2026

Black Hole Properties of Type-1 Active Galactic Nuclei in the North Ecliptic Pole Wide Field: I. Mid-infrared Sources with Optical Counterparts

Dohyeong Kim, Myungshin Im, Hyunjin Shim +11

We present measurements of black hole (BH) properties of 861 Type-1 active galactic nuclei (AGNs) in the North Ecliptic Pole (NEP)-Wide field. These AGNs are detected in both optic…

astro-ph.GA2025

The Redshifts from 122 Bands: Comparative Redshift Forecast for Low-Resolution Spectra from SPHEREx and 7-Dimensional Sky Survey (7DS)

Jangho Bae, Bomee Lee, Myungshin Im +21

The recently initiated SPHEREx and 7DS surveys will deliver low-resolution spectra () for hundreds of millions of galaxies over the optical to near-infrared range…

astro-ph.EP2025

Optical and Near-Infrared Contemporaneous Polarimetry of C/2023 A3 (Tsuchinshan-ATLAS)

Bumhoo Lim, Masateru Ishiguro, Jun Takahashi +11

We conducted contemporaneous optical and near-infrared polarimetric and spectroscopic observations of C/2023 A3 (Tsuchinshan-ATLAS, hereafter T-A) from 2024 October 16 to December…

astro-ph.GA2025

JWST Spectroscopic View of a Rapidly Growing Dust-obscured Quasar at : Effect of Dust Extinction Correction on Black Hole Mass and Eddington Ratio Estimation

Dohyeong Kim, Myungshin Im

In the merger-driven galaxy evolution scenario, the central supermassive black holes (SMBHs) in dust obscured galaxies grow rapidly. Interestingly, a recent work \citep{suh24} on a…

astro-ph.GA2024

Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field

Eunhee Ko, Myungshin Im, Seong-Kook Lee +1

It is yet to be understood how large-scale environments influence star formation activity in galaxy clusters. One recently proposed mechanism is that galaxy clusters can remain sta…