most citedLong Plateau Doth So: How Internal Heating Sources Affect Hydrogen-Rich Supernova Light Curves

2 citations · 3 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2025

Formation of circumstellar material during double-white-dwarf mergers and the early excess emissions in Type Ia supernovae

Yusuke Inoue, Keiichi Maeda, Takashi Nagao +1

Early excess emission observed in Type Ia supernovae (SNe Ia) within day of explosion provides a critical window into their progenitor systems. In the present study, we inv…

astro-ph.HE2024

Probing the Origin of the Star Formation Excess Discovered by JWST through Gamma-Ray Bursts

Tatsuya Matsumoto, Yuichi Harikane, Keiichi Maeda +1

The recent observations by the James Webb Space Telescope (JWST) have revealed a larger number of bright galaxies at than was expected. The origin of this excess is st…

astro-ph.HE2024★ 1 cited

Diversity in hydrogen-rich envelope mass of type II supernovae (II): SN 2023ixf as explosion of partially-stripped intermediate massive star

Qiliang Fang, Takashi J. Moriya, Lucía Ferrari +6

SN 2023ixf is one of the most well-observed core-collapse supernova in recent decades, yet there is inconsistency in the inferred zero-age-main-sequence (ZAMS) mass …

astro-ph.HE2024

Diversity in hydrogen-rich envelope mass of type II supernovae (I): -band light curve modeling

Qiliang Fang, Keiichi Maeda, Haonan Ye +2

We present a systematic study of Type II supernovae (SNe II) originating from progenitors with effective temperatures () and luminosities closely resembling red superg…

astro-ph.HE2024★ 2 cited

Long Plateau Doth So: How Internal Heating Sources Affect Hydrogen-Rich Supernova Light Curves

Tatsuya Matsumoto, Brian D. Metzger, Jared A. Goldberg

Some hydrogen-rich core-collapse supernovae (type IIP SNe) exhibit evidence for a sustained energy source powering their light curves, resulting in a brighter and/or longer-lasting…