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researcher

Shao-Ming Hu

18 papers hereh-index 00 citations0 works total

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

author position
  • first author2
  • middle author15

Across the 17 of 18 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE8
  • astro-ph.SR5
  • astro-ph.IM3
  • astro-ph.EP2
same name
  • Shao-Ming Hu — 5 papers, h 7
  • Shao-Ming Hu — 3 papers, h 3
  • Shao-Ming Hu — 1 paper, h 1

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
20132022
most citedGaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy

81 citations · 324 across the 18 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

1 paper · 2 filters

astro-ph.HE2017★ 81 cited

Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy

Subhash Bose, Subo Dong, A. Pastorello +55

Hydrogen-poor superluminous supernovae (SLSNe-I) have been predominantly found in low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an SLSN-I o…

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