activity
20242026
collaborators

6 papers

astro-ph.HE2026

The environmental dependence of mid-IR luminous dusty Supernovae

Lin Xiao, Zeyue Peng, Lluis Galbany +10

Using the Spitzer and WISE images, we discovered 42 mid-IR luminous dusty supernovae with local integral-field spectroscopy data. The observed mid-IR emission indicates the presenc…

astro-ph.GA2025

A candidate for True Type-2 AGN without hidden central BLRs Identified by central Tidal Disruption Event

Gu Ying, Zheng Qi, Cheng Peizheng +4

In this manuscript, through applications of TDE (tidal disruption event) expected variability properties, a potential candidate for True type-2 AGN without hidden central broad lin…

astro-ph.SR2025

Very Late-Time JWST and Keck Spectra of the Oxygen-Rich Supernova 1995N

Geoffrey C. Clayton, R. Wesson, Ori D. Fox +43

We present new {\it JWST}/MIRI MRS and Keck spectra of SN 1995N obtained in 2022--2023, more than 10,000 days after the supernova (SN) explosion. These spectra are among the latest…

astro-ph.SR2025

JWST/MIRI detects the dusty SN1993J about 30 years after explosion

Tamás Szalai, Szanna Zsíros, Jacob Jencson +37

Core-collapse supernovae (CCSNe) have long been considered to contribute significantly to the cosmic dust budget. New dust cools quickly and is therefore detectable at mid-infrared…

astro-ph.SR2024

Mass Ratio Distribution of Hierarchical Triple Systems from the LAMOST-MRS Survey

Tongyu He, Jiangdan Li, Xuefei Chen +3

Hierarchical triple-star systems consists of three components organised into an inner binary (,) and a more distant outer tertiary () star. The LAMOST Medium-R…

astro-ph.HE2024

JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip

Melissa Shahbandeh, Ori D. Fox, Tea Temim +42

Dust from core-collapse supernovae (CCSNe), specifically Type IIP SNe, has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject lar…