D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 73 Citations 16,133 203 World Ranking 2807 National Ranking 262

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Galaxy

Sean G. Ryan mostly deals with Astrophysics, Stars, Astronomy, Nucleosynthesis and Metallicity. His Spectral line research extends to Astrophysics, which is thematically connected. The study incorporates disciplines such as Spectroscopy, Supernova and Equivalent width in addition to Stars.

He does research in Astronomy, focusing on Milky Way specifically. His Nucleosynthesis course of study focuses on Subgiant and Stellar mass, Giant star, Stellar nucleosynthesis, Star formation and K-type main-sequence star. The concepts of his Metallicity study are interwoven with issues in Halo and Galaxy formation and evolution.

His most cited work include:

  • The Gaia-ESO Public Spectroscopic Survey (516 citations)
  • Nucleosynthetic signatures of the first stars (512 citations)
  • Extremely Metal-Poor Stars. II. Elemental Abundances and the Early Chemical Enrichment of The Galaxy* (468 citations)

What are the main themes of his work throughout his whole career to date?

Sean G. Ryan mainly focuses on Astrophysics, Stars, Astronomy, Nucleosynthesis and Metallicity. In general Astrophysics study, his work on Galaxy, Galactic halo and Halo often relates to the realm of Population, thereby connecting several areas of interest. Sean G. Ryan works mostly in the field of Galaxy, limiting it down to topics relating to Equivalent width and, in certain cases, Diffuse interstellar band.

Within one scientific family, Sean G. Ryan focuses on topics pertaining to Supernova under Stars, and may sometimes address concerns connected to Cosmic ray. His research in Nucleosynthesis intersects with topics in Subgiant, Abundance of the chemical elements and Radial velocity. His studies in Spectral line integrate themes in fields like Line and Atomic physics.

He most often published in these fields:

  • Astrophysics (89.76%)
  • Stars (74.41%)
  • Astronomy (47.24%)

What were the highlights of his more recent work (between 2008-2021)?

  • Astrophysics (89.76%)
  • Stars (74.41%)
  • Nucleosynthesis (32.28%)

In recent papers he was focusing on the following fields of study:

Sean G. Ryan spends much of his time researching Astrophysics, Stars, Nucleosynthesis, Astronomy and Galaxy. Sean G. Ryan performs multidisciplinary study in Astrophysics and Population in his work. In the field of Stars, his study on Metallicity and Stellar atmosphere overlaps with subjects such as Metal.

His Nucleosynthesis research incorporates themes from Spectral line, Abundance of the chemical elements and Spectroscopy. His research on Astronomy often connects related areas such as Neutron capture. In general Galaxy, his work in Halo, Quasar and Diffuse interstellar band is often linked to Thermodynamic equilibrium and Organic molecules linking many areas of study.

Between 2008 and 2021, his most popular works were:

  • The Gaia-ESO Public Spectroscopic Survey (516 citations)
  • THE MOST METAL-POOR STARS. II. CHEMICAL ABUNDANCES OF 190 METAL-POOR STARS INCLUDING 10 NEW STARS WITH [Fe/H] ⩽ –3.5*, **, ** * (262 citations)
  • The Most Metal-poor Stars. IV. The Two Populations with [Fe/H] ?3.0 (185 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Milky Way
  • Galaxy

Sean G. Ryan mainly investigates Astrophysics, Stars, Nucleosynthesis, Astronomy and Abundance of the chemical elements. His studies link Spectrograph with Astrophysics. His Stars study incorporates themes from William Herschel Telescope and Wavelength range.

His Nucleosynthesis study integrates concerns from other disciplines, such as Spectroscopy, Spectral line, Stellar atmosphere, Subgiant and Star. His work in Milky Way and Galactic halo is related to Astronomy. In his work, Giant star is strongly intertwined with Stellar evolution, which is a subfield of Abundance of the chemical elements.

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

The Gaia-ESO Public Spectroscopic Survey

G. Gilmore;S. Randich;M. Asplund;J. Binney.
The Messenger (2012)

1036 Citations

Extremely Metal-Poor Stars. II. Elemental Abundances and the Early Chemical Enrichment of The Galaxy*

Sean G. Ryan;John E. Norris;Timothy C. Beers.
The Astrophysical Journal (1996)

786 Citations

Nucleosynthetic signatures of the first stars

Anna Frebel;Wako Aoki;Norbert Christlieb;Hiroyasu Ando.
Nature (2005)

704 Citations

Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars*

Wako Aoki;Timothy C. Beers;Norbert Christlieb;John E. Norris.
The Astrophysical Journal (2007)

669 Citations

Primordial Lithium and Big Bang Nucleosynthesis.

Sean G. Ryan;Timothy C. Beers;Keith A. Olive;Brian D. Fields.
The Astrophysical Journal (2000)

433 Citations

The Spite Lithium Plateau: Ultrathin but Postprimordial

Sean G. Ryan;John E. Norris;Timothy C. Beers.
The Astrophysical Journal (1999)

389 Citations

The Spite Lithium Plateau: Ultra-Thin but Post-Primordial

Sean G. Ryan;John E. Norris;Timothy C. Beers.
arXiv: Astrophysics (1999)

362 Citations

EXTREMELY METAL-POOR STARS. VIII. HIGH-RESOLUTION, HIGH SIGNAL-TO-NOISE RATIO ANALYSIS OF FIVE STARS WITH (Fe/H) ( (3.5

John E. Norris;Sean G. Ryan;Timothy C. Beers.
The Astrophysical Journal (2001)

349 Citations

The Binary Frequency Among Carbon-enhanced, s-Process-rich, Metal-poor Stars

Sara Lucatello;Sara Lucatello;Stelios Tsangarides;Timothy C. Beers;Eugenio Carretta.
The Astrophysical Journal (2005)

342 Citations

Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

John E. Norris;Sean G. Ryan;Timothy C. Beers.
arXiv: Astrophysics (2001)

330 Citations

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