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researcher

Xiaofeng Wang

112 papers hereh-index 355.1k citations269 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author7
  • middle author84
  • last author10

Across the 101 of 112 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE57
  • astro-ph.SR27
  • astro-ph11
  • astro-ph.CO7
  • astro-ph.IM7
  • astro-ph.EP1
same name
  • Xiaofeng Wang — 37 papers, h 39
  • Xiaofeng Wang — 37 papers, h 12
  • Xiaofeng Wang — 32 papers, h 6
  • Xiaofeng Wang — 30 papers, h 11
  • Xiaofeng Wang — 20 papers, h 61
  • Xiaofeng Wang — 12 papers, h 10

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20042023
most citedNearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample

823 citations · 6.3k across the 111 of their papers we have counts for

collaborators
Showing 2007Show all

3 papers · 1 filter

astro-ph2007★ 92 cited

The Detection of a Light Echo from the Type Ia Supernova 2006X in M100

Xiaofeng Wang, Weidong Li, Alexei V. Filippenko +3

We report the discovery of a light echo (LE) from the Type Ia supernova (SN) 2006X in the nearby galaxy M100. The presence of the LE is supported by analysis of both the Advanced C…

astro-ph2007★ 199 cited

Optical and Near-Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova 2006X in M100

Xiaofeng Wang, Weidong Li, Alexei V. Filippenko +14

We present extensive optical (UBVRI), near-infrared (JK) light curves and optical spectroscopy of the Type Ia supernova (SN) 2006X in the nearby galaxy NGC 4321 (M100). Our observa…

astro-ph2007★ 28 cited

Distribution of 56Ni Yields of Type Ia Supernovae and its Implication for Progenitors

Bo Wang, Xiangcun Meng, Xiaofeng Wang +1

The amount of 56Ni produced in type Ia supernova (SN Ia) explosion is probably the most important physical parameter underlying the observed correlation of SN Ia luminosities…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.