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20242026
most citedDetection of [C I] Emission in Nebular Spectra of a Peculiar Type Ia Supernova 2022pul

5 citations · 9 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group

Danfeng Xiang, Xiaofeng Wang, Jujia Zhang +40

The extent of envelope stripping in the progenitor stars is directly reflected in the diversity of spectral features observed in stripped-envelope supernovae (SESNe). Through exten…

astro-ph.SR20254 cited

An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi

Yi Yang, Xudong Wen, Lifan Wang +18

The death of massive stars is triggered by an infall-induced bounce shock that disrupts the star. How such a shock is launched and propagates through the star is a decade-long puzz…

astro-ph.HE2025

Supernovae at Distances < 40 Mpc: II. Supernova Rate in the Local Universe

Xiaoran Ma, Xiaofeng Wang, Jun Mo +21

Context.This is the second paper of a series aiming to determine the birth rates of supernovae in the local Universe. Aims. In this paper, we aim to estimate the SN rates in the lo…

astro-ph.HE2025

Supernovae at Distances < 40 Mpc: I.Catalogues and fractions of Supernovae in a Complete Sample

Xiaoran Ma, Xiaofeng Wang, Jun Mo +20

Context.This is the first paper of a series aiming to determine the fractions and birth rates of various types of supernovae (SNe) in the local Universe. Aims. In this paper, we ai…

astro-ph.HE2025

Optical and Near-infrared Observations of SN 2023ixf for over 600 days after the Explosion

Gaici Li, Xiaofeng Wang, Yi Yang +37

Context.We present a comprehensive photometric and spectroscopic study of the nearby Type II supernova (SN) 2023ixf, with our extensive observations spanning the phases from ~3 to…

astro-ph.HE20255 cited

Detection of [C I] Emission in Nebular Spectra of a Peculiar Type Ia Supernova 2022pul

Jialian Liu, Xiaofeng Wang, Yi Yang +6

SN 2022pul gains special attention due to its possible origin of a super-Chandarsekhar-mass white dwarf explosion (or called a 03fg-like type Ia supernova), which shows prominent […