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20152023
most citedEnergetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star

148 citations · 714 across the 28 of their papers we have counts for

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18 papers · 1 filter

astro-ph.HE2023

Implications for the Explosion Mechanism of Type Ia Supernovae from their Late-time Spectra

Jialian Liu, Xiaofeng Wang, Alexei V. Filippenko +10

Late-time spectra of Type Ia supernovae (SNe Ia) are important in clarifying the physics of their explosions, as they provide key clues to the inner structure of the exploding whit…

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.HE2022★ 14 cited

The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event

Yi Yang, Dietrich Baade, Peter Hoeflich +29

A rare class of supernovae (SNe) is characterized by strong interaction between the ejecta and several solar masses of circumstellar matter (CSM) as evidenced by strong Balmer-line…

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★ 29 cited

Observations of the Very Young Type Ia Supernova 2019np with Early-excess Emission

Hanna Sai, Xiaofeng Wang, Nancy Elias-Rosa +30

Early-time radiative signals from type Ia supernovae (SNe Ia) can provide important constraints on the explosion mechanism and the progenitor system. We present observations and an…

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.HE2021★ 16 cited

SN 2018agk: A Prototypical Type Ia Supernova with a Smooth Power-law Rise in Kepler (K2)

Qinan Wang, Armin Rest, Yossef Zenati +73

We present the 30-min cadence Kepler/K2 light curve of the Type Ia supernova (SN Ia) SN 2018agk, covering approximately one week before explosion, the full rise phase and the decli…

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

Optical and Ultraviolet Monitoring of the Black Hole X-ray Binary MAXI J1820+070/ASASSN-18ey for 18 Months

Hanna Sai, Xiaofeng Wang, Jianfeng Wu +20

MAXI J1820+070 is a low-mass black hole X-ray binary system with high luminosity in both optical and X-ray bands during the outburst periods. We present extensive photometry in X-r…

astro-ph.HE2021★ 8 cited

SN 2017hpa: A Nearby Carbon-Rich Type Ia Supernova with a Large Velocity Gradient

Xiangyun Zeng, Xiaofeng Wang, Ali Esamdin +24

We present extensive, well-sampled optical and ultraviolet photometry and optical spectra of the Type Ia supernova (SN Ia) 2017hpa. The light curves indicate that SN 2017hpa is a n…

astro-ph.HE2021★ 40 cited

The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

Danfeng Xiang, Xiaofeng Wang, Weili Lin +47

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to 70 days and the spectroscopy rang…

astro-ph.HE2020★ 19 cited

Optical and Near-Infrared Observations of the Nearby Type Ia Supernova 2017cbv

Lingzhi Wang, Carlos Contreras, Maokai Hu +28

Supernova (SN) 2017cbv in NGC 5643 is one of a handful of type Ia supernovae (SNe~Ia) reported to have excess blue emission at early times. This paper presents extensive $BVRIYJHK_…

astro-ph.HE2018★ 42 cited

The Cold and Dusty Circumstellar Matter around Fast-expanding Type Ia Supernovae

Xiaofeng Wang, Jia Chen, Lifan Wang +5

Type Ia supernovae (SNe Ia) play key roles in revealing the accelerating expansion of the universe, but our knowledge about their progenitors is still very limited. Here we report…

astro-ph.HE2018★ 87 cited

Seeing Double: ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve

B. J. Shappee, T. W. -s. Holoien, M. R. Drout +109

On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnit…

astro-ph.HE2018★ 15 cited

Optical Observations of the Young Type Ic Supernova SN 2014L in M99

Jujia Zhang, Xiaofeng Wang, József Vinkó +22

We present optical spectroscopic and photometric observations of the nearby type Ic supernova (SN Ic) SN 2014L. This SN was discovered by the Tsinghua-NAOC Transient Survey (TNTS)…

astro-ph.HE2018★ 15 cited

Optical Observations of the 2002cx-like Supernova 2014ek, and Characterizations of SNe Iax

Linyi Li, Xiaofeng Wang, Jujia Zhang +14

We present optical observations of supernova (SN) 2014ek discovered during the Tsinghua-NAOC Transient Survey (TNTS), which shows properties that are consistent with those of SN 20…

astro-ph.HE2017★ 148 cited

Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star

Iair Arcavi, D. Andrew Howell, Daniel Kasen +50

Every supernova hitherto observed has been considered to be the terminal explosion of a star. Moreover, all supernovae with absorption lines in their spectra show those lines decre…

astro-ph.HE2016★ 99 cited

Optical Observations of the Type Ia Supernova 2011fe in M101 for Nearly 500 Days

Kaicheng Zhang, Xiaofeng Wang, JuJia Zhang +17

We present well-sampled optical observations of the bright Type Ia supernova (SN~Ia) SN 2011fe in M101. Our data, starting from days before maximum light and extending to…