arrow
Y

Yize Dong

center for astrophysics harvard & smithsonian
H指数:19
被引数:1,096

个人简介

暂无内容

教育背景

暂无内容

工作经历

暂无内容

荣誉奖项

暂无内容

SN 2022xus: bridging the gap between Type IIP and IIL supernovae

SN 2022xus: 连接IIP型与IIL型超新星之间的桥梁

2026-08-030
OAAI
SN 2024abfl: A Flat-plateau; Low-luminosity Type IIP Supernova with Early Circumstellar Matter Interaction

SN 2024abfl:一颗具有平坦平台、低光度IIP型超新星,且早期存在 circumstellar matter 相互作用

2026-04-270
OAAI
Photometry and Spectroscopy of SN 2024pxl: A Luminosity Link among Type Iax Supernovae

光度学和光谱学观测 SN 2024pxl:Iax 型超新星的光度关联

2026-03-090
OAAI
SN 2023zcu: A Type IIP SN with Early Flash Features

SN 2023zcu: 一颗具有早期闪光特征的IIP型超新星

2026-02-250
OAAI
The First Radio View of a Type Ibn Supernova in SN 2023fyq: Understanding the Mass-loss History in the Last Decade before the Explosion

SN 2023fyq型Ibn超新星的首例射电观测:理解爆炸前最后十年中的质量损失历史

2025-12-120
OAAI
Mid-infrared Dust Evolution and Late-time Circumstellar Medium Interaction in SN 2017eaw

中红外尘埃演化及SN 2017eaw晚期星周介质相互作用

2025-11-050
OA
SN 2019hnl: A Type IIP Supernova with a Partially Stripped; Low-mass Progenitor

SN 2019hnl:一颗具有部分被剥离、低质量原初恒星的IIP型超新星

2025-10-220
OAAI
Early Shock Cooling Observations and Progenitor Constraints of Type IIb Supernova SN 2024uwq

早期冲击冷却观测与IIb型超新星SN 2024uwq的前身星约束

2025-09-100
OA
JWST and Ground-based Observations of the Type Iax Supernovae SN 2024pxl and SN 2024vjm: Evidence for Weak Deflagration Explosions

JWST与地面观测到的Iax型超新星SN 2024pxl和SN 2024vjm:弱爆燃爆炸的证据

2025-08-130
PRE
A Multiwavelength Autopsy of the Interacting Type IIn Supernova 2020ywx: Tracing Its Progenitor Mass-loss History for 100 Yr Before Death

多波段分析相互作用型IIn超新星2020ywx:追溯其死亡前100年母体质量损失历史

2025-04-110
OA
SN 2018is: A low-luminosity Type IIP supernova with narrow hydrogen emission lines at early phases
2025-02-190
OA
SN2023fyq: A Type Ibn Supernova with Long-standing Precursor Activity Due to Binary Interaction
2024-12-180
OA
A JWST Medium-resolution MIRI Spectrum and Models of the Type Ia Supernova 2021aefx at+415 days
2024-11-040
OA
Characterizing the Rapid Hydrogen Disappearance in SN 2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
2024-10-180
OA
Circumstellar Interaction in the Ultraviolet Spectra of SN 2023ixf 14-66 Days After Explosion
2024-09-242
OA
Extended Shock Breakout and Early Circumstellar Interaction in SN 2024ggi
2024-08-262
OA
Circumstellar Interaction Signatures in the Low-luminosity Type II SN 2021gmj
2024-08-131
OA
Ground-based and JWST Observations of SN 2022pul. II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type Ia Supernova
2024-04-305
OA