activity
20122024
most citedEnergetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star

148 citations · 1.9k across the 62 of their papers we have counts for

collaborators

62 papers

astro-ph.HE2024★ 29 cited

Probing the Shock Breakout Signal of SN 2024ggi from the Transformation of Early Flash Spectroscopy

Jujia Zhang, Luc Dessart, Xiaofeng Wang +11

We present early-time, hour-to-day cadence spectroscopy of the nearby type II supernova (SN II) 2024ggi, which was discovered at a phase when the SN shock just emerged from the red…

astro-ph.HE2024

SN 2021dbg: A Luminous Type IIP-IIL Supernova Exploding from a Massive Star with a Layered Shell

Zeyi Zhao, Jujia Zhang, Liping Li +9

We present extensive observations and analysis of supernova (SN) 2021dbg, utilizing optical photometry and spectroscopy. For approximately 385 days following the explosion, SN 2021…

astro-ph.HE2024

The Red Supergiant Progenitor of Type II Supernova 2024ggi

Danfeng Xiang, Jun Mo, Xiaofeng Wang +8

We present a detailed analysis of the progenitor and its local environment for the recently discovered type II supernova (SN) 2024ggi at a distance of about 6.7~Mpc, by utilizing t…

astro-ph.HE2024

Extended Shock Breakout and Early Circumstellar Interaction in SN 2024ggi

Manisha Shrestha, K. Azalee Bostroem, David J. Sand +40

We present high-cadence photometric and spectroscopic observations of supernova (SN) 2024ggi, a Type II SN with flash spectroscopy features which exploded in the nearby galaxy NGC…

astro-ph.HE2024

Probing diversity of type II supernovae with the Chinese Space Station Telescope

Han Lin, Jujia Zhang, Xinghan Zhang

Type II supernovae (SNe II), which show abundant hydrogen in their spectra, belong to a class of SNe with diverse observed properties. It is commonly accepted that SNe II are produ…

astro-ph.HE2023★ 73 cited

A Shock Flash Breaking Out of a Dusty Red Supergiant

Gaici Li, Maokai Hu, Wenxiong Li +41

Shock breakout emission is light that arises when a shockwave, generated by core-collapse explosion of a massive star, passes through its outer envelope. Hitherto, the earliest det…

astro-ph.SR2023★ 37 cited

The Dusty and Extremely Red Progenitor of the Type II Supernova 2023ixf in Messier 101

Danfeng Xiang, Jun Mo, Lingzhi Wang +4

Stars with initial masses in the range of 8-25 solar masses are thought to end their lives as hydrogen-rich supernovae (SNe II). Based on the pre-explosion images of Hubble Space T…

astro-ph.HE2023★ 37 cited

Circumstellar Material Ejected Violently by A Massive Star Immediately before its Death

Jujia Zhang, Han Lin, Xiaofeng Wang +7

Type II supernovae represent the most common stellar explosions in the Universe, for which the final stage evolution of their hydrogen-rich massive progenitors towards core-collaps…

astro-ph.HE2023

Discovery of the Closest Ultrastripped Supernova: SN 2021agco in UGC 3855

Shengyu Yan, Xiaofeng Wang, Xing Gao +16

We present the discovery and studies of the helium-rich, fast-evolving supernova (SN) 2021agco at a distance of 40 Mpc. Its early-time flux is found to rise from half peak t…

astro-ph.HE2023★ 3 cited

Newly Formed Dust within the Circumstellar Environment of SNIa-CSM 2018evt

Lingzhi Wang, Maokai Hu, Lifan Wang +44

Dust associated with various stellar sources in galaxies at all cosmic epochs remains a controversial topic, particularly whether supernovae (SNe) play an important role in dust pr…

astro-ph.HE2023

SN 2022vqz: A Peculiar Subluminous Type Ia Supernova with Prominent Early Excess Emission

Gaobo Xi, Xiaofeng Wang, Gaici Li +22

We present extensive photometric and spectroscopic observations of the peculiar Type Ia supernova (SN Ia) 2022vqz. It shares many similarities with the SN 2002es-like SNe Ia, such…

astro-ph.HE2023★ 6 cited

SN 2016ije: An SN 2002es-like Type Ia Supernova Exploded in a Metal-poor and Low-surface Brightness Galaxy

Zhitong Li, Tianmeng Zhang, Xiaofeng Wang +28

We have conducted photometric and spectroscopic observations of the peculiar Type Ia supernova (SN Ia) 2016ije that was discovered through the Tsinghua-NAOC Transient Survey. This…

astro-ph.HE2023★ 12 cited

SN 2018hna: Adding a Piece to the Puzzles of the Explosion of Blue Supergiants

Danfeng Xiang, Xiaofeng Wang, Xinghan Zhang +14

We present extensive optical/ultraviolet observations and modelling analysis for the nearby SN 1987A-like peculiar Type II supernova (SN) 2018hna. Both photometry and spectroscopy…

astro-ph.HE2022★ 8 cited

SN 2019ein: A Type Ia Supernova Likely Originated from a Sub-Chandrasekhar-Mass Explosion

Gaobo Xi, Xiaofeng Wang, Wenxiong Li +12

We present extensive optical photometric and spectroscopic observations for the nearby Type Ia supernova (SN Ia) 2019ein, spanning the phases from days to days…

astro-ph.HE2022★ 6 cited

AT2021acak: a candidate tidal disruption event found in the Zwicky Transient Facility survey

Jie Li, Zhongxiang Wang, Dong Zheng +3

We report a candidate tidal disruption event (TDE) found in the Zwicky Transient Facility (ZTF) survey data. This candidate, with its transient name AT2021acak, showed brightness i…

astro-ph.HE2022

SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve

Xinghan Zhang, Xiaofeng Wang, Hanna Sai +12

We present multi-band photometric and spectroscopic observations of the type II supernova, (SN) 2019va, which shows an unusually flat plateau-phase evolution in its V-band light cu…

astro-ph.HE2022★ 12 cited

Evolution of A Peculiar Type Ibn Supernova SN 2019wep

Anjasha Gangopadhyay, Kuntal Misra, Griffin Hosseinzadeh +14

We present a high-cadence short term photometric and spectroscopic monitoring campaign of a type Ibn SN 2019wep, which is one of the rare SN Ibn after SNe 2010al and 2019uo to disp…

astro-ph.HE2022★ 16 cited

SN 2012ij: A low-luminosity type Ia supernova and evidence for continuous distribution from 91bg-like explosion to normal ones

Zhitong Li, Tianmeng Zhang, Xiaofeng Wang +24

In this paper, we present photometric and spectroscopic observations of a subluminous type Ia supernova (SN Ia) 2012ij, which has an absolute -band peak magnitude $M_{B,\rm{max}…

astro-ph.HE2021

SN 2018hfm : A Low-Energy Type II Supernova with Prominent Signatures of Circumstellar Interaction and Dust Formation

Xinghan Zhang, Xiaofeng Wang, Hanna Sai +13

We present multiband optical photometric and spectroscopic observations of an unusual Type II supernova, SN 2018hfm, which exploded in the nearby (d = 34.67 Mpc) dwarf galaxy PGC 1…

astro-ph.HE2021★ 10 cited

SN 2015bq: A Luminous Type Ia Supernova with Early Flux Excess

Liping Li, Jujia Zhang, Benzhong Dai +4

We present optical and ultraviolet (UV) observations of a luminous type Ia supernova (SN Ia) SN 2015bq characterized by the early flux excess. This SN reaches a B-band absolute mag…

astro-ph.SR2021★ 9 cited

SN 2021csp -- the explosion of a stripped envelope star within a H and He-poor circumstellar medium

Morgan Fraser, Maximilian D. Stritzinger, Sean J. Brennan +48

We present observations of SN 2021csp, a unique supernova (SN) which displays evidence for interaction with H- and He- poor circumstellar material (CSM) at early times. Using high-…

astro-ph.HE2021★ 1 cited

SN 2017fgc: A Fast-Expanding Type Ia Supernova Exploded in Massive Shell Galaxy NGC 474

Xiangyun Zeng, Xiaofeng Wang, Ali Esamdin +31

We present extensive optical photometric and spectroscopic observations of the high-velocity (HV) Type Ia supernova (SN Ia) 2017fgc, covering the phase from 12 d before to $…

astro-ph.HE2021★ 8 cited

ASASSN-14ms:the Most Energetic Known Explosion of a Type Ibn Supernova and its Physical Origin

Xiaofeng Wang, Weili Lin, Jujia Zhang +14

ASASSN-14ms may represent the most luminous Type Ibn supernova (SN~Ibn) ever detected, with an absolute U-band magnitude brighter than -22.0 mag and a total bolometric luminosity >…

astro-ph.HE2021

SN 2015bf: a fast declining type II supernova with flash-ionised signatures

Han Lin, Xiaofeng Wang, Jujia Zhang +19

We present optical and ultraviolet photometry, as well as optical spectra, for the type II supernova (SN) 2015bf. Our observations cover the phases from to d af…