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researcher

G. Clayton

11 papers hereh-index 10650 citations22 works total

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

author position
  • middle author10

Across the 10 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR8
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • G. Clayton — 110 papers, h 45
  • G. Clayton — 10 papers, h 5
  • G. Clayton — 3 papers, h 1
  • G. Clayton — 2 papers, h 3
  • G. Clayton — 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
20112024
most citedThe Dust Budget of the SMC: Are AGB Stars the Primary Dust Source at Low Metallicity?

149 citations · 309 across the 11 of their papers we have counts for

collaborators
Showing 2022Show all

2 papers · 1 filter

astro-ph.SR2022★ 2 cited

Quantifying the dust in SN 2012aw and iPTF14hls with ORBYTS

Maria Niculescu-Duvaz, M. J. Barlow, W. Dunn +32

Core-collapse supernovae (CCSNe) are potentially capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended pe…

astro-ph.SR2022★ 33 cited

Dust masses for a large sample of core-collapse supernovae from optical emission line asymmetries: dust formation on 30-year timescales

Maria Niculescu-Duvaz, Michael J Barlow, Antonia Bevan +7

Modelling the red-blue asymmetries seen in the broad emission lines of core-collapse supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta at…

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