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Sean G. Ryan

12 papers hereh-index 11759 citations16 works total

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

author position
  • middle author5
  • last author4

Across the 9 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.GA4
  • astro-ph.SR3
  • astro-ph.CO1
same name
  • Sean G. Ryan — 1 paper

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
20022015
most citedThe Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] < -3.0

217 citations · 855 across the 12 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2012★ 217 cited

The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] < -3.0

John E. Norris, David Yong, M. S. Bessell +8

We discuss the carbon-normal and carbon-rich populations of Galactic halo stars having [Fe/H] < -3.0, utilizing chemical abundances from high-resolution, high-S/N model-atmosphere…

astro-ph.GA2012★ 131 cited

The Most Metal-Poor Stars. III. The Metallicity Distribution Function and CEMP Fraction

David Yong, John E. Norris, M. S. Bessell +6

We examine the metallicity distribution function (MDF) and fraction of carbon-enhanced metal-poor (CEMP) stars in a sample that includes 86 stars with [Fe/H] < -3.0, based on high-…

astro-ph.GA2012★ 78 cited

The Most Metal-Poor Stars. I. Discovery, Data, and Atmospheric Parameters

John E. Norris, M. S. Bessell, David Yong +7

We report the discovery of 34 stars in the Hamburg/ESO Survey for metal-poor stars and the Sloan Digital Sky Survey that have [Fe/H] < -3.0. Their median and minimum abundances are…

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