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Ken W. Smith

4 papers hereh-index 4189 citations5 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.SR1
same name
  • Ken W. Smith — 7 papers, h 8
  • Ken W. Smith — 7 papers, h 2
  • Ken W. Smith — 4 papers, h 1
  • Ken W. Smith — 4 papers, h 1
  • Ken W. Smith — 1 paper, h 2

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
20152026
most citedType Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light

129 citations · 267 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2026

Decadal pre-explosion activity and circumstellar interaction in a supernova

Ting-Wan Chen, Amar Aryan, Sheng Yang +52

When a massive star explodes as a supernova, crucial information about its immediate environment is lost within hours. Here we report rapid optical observations from Lulin Observat…

astro-ph.HE2016★ 129 cited

Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light

Griffin Hosseinzadeh, Iair Arcavi, Stefano Valenti +34

Type Ibn supernovae (SNe) are a small yet intriguing class of explosions whose spectra are characterized by low-velocity helium emission lines with little to no evidence for hydrog…

astro-ph.HE2015★ 93 cited

Measuring nickel masses in Type Ia supernovae using cobalt emission in nebular phase spectra

Michael J. Childress, D. John Hillier, Ivo Seitenzahl +34

The light curves of Type Ia supernovae (SNe Ia) are powered by the radioactive decay of 56Ni to 56Co at early times, and the decay of 56Co to 56Fe from ~60 days…

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