activity
20042026
most citedUWISH2 -- The UKIRT Widefield Infrared Survey for H2

77 citations · 339 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2026

A Comparative Study of the Supernova Remnant Cassiopeia A from 2013--2020 Deep [Fe II]+[Si I] Images

Seung-Hoon Jung, Bon-Chul Koo, Yong-Hyun Lee +2

We present a comparative analysis of supernova remnant Cassiopeia A based on two deep, narrow-band images covering the [Fe II] 1.644um + [Si I] 1.645um lines obtained in 2013 and 2…

astro-ph.GA2026★ 3 cited

Extended Ionized Fe Objects in the UWIFE Survey

Kim Yesol, Koo Bon-Chul, Pyo Tae-Soo +7

We explore systematically the shocked gas in the first Galactic quadrant of the Milky Way using the United Kingdom Infrared Telescope (UKIRT) Wide-field Infrared Survey for Fe+ (UW…

astro-ph.GA2025

Near-infrared [P II] and [Fe II] line mapping of Galactic supernova remnants

Takuma Kokusho, Yuki Katsurada, Yong-Hyun Lee +7

Phosphorus (P) is one of the key ingredients for life, yet its origins in galaxies remain poorly understood. In order to investigate the production of P by supernovae, we performed…

astro-ph.HE2024★ 51 cited

A JWST Survey of the Supernova Remnant Cassiopeia A

Dan Milisavljevic, Tea Temim, Ilse De Looze +43

We present initial results from a JWST survey of the youngest Galactic core-collapse supernova remnant Cassiopeia A (Cas A), made up of NIRCam and MIRI imaging mosaics that map emi…

astro-ph.GA2023★ 2 cited

Supernova Ejecta with Crystalline Silicate Dust in the Supernova Remnant MSH 15-52

Hyun-Jeong Kim, Bon-Chul Koo, Takashi Onaka

IRAS 15099-5856 in the young supernova remnant (SNR) MSH 15-52 is the first and only SNR-associated object with crystalline silicate dust detected so far, although its nature and t…

astro-ph.GA2019★ 18 cited

Revealing The CO X-factor In Dark Molecular Gas through Sensitive ALMA Absorption Observations

Gan Luo, Di Li, Ningyu Tang +11

Carbon-bearing molecules, particularly CO, have been widely used as tracers of molecular gas in the interstellar medium (ISM). In this work, we aim to study the properties of molec…