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researcher

R. Mathieu

82 papers hereh-index 548.2k citations275 works total

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

author position
  • sole author1
  • first author4
  • middle author50
  • last author23

Across the 78 of 82 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR55
  • astro-ph27
same name
  • R. Mathieu — 47 papers, h 34
  • R. Mathieu — 4 papers, h 4
  • R. Mathieu — 3 papers, h 2
  • R. Mathieu — 1 paper
  • R. Mathieu — 1 paper, h 3
  • R. Mathieu — 1 paper, h 0

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
19942023
most citedA Robust Measure of Tidal Circularization in Coeval Binary Populations: The solar-type spectroscopic Binary Population in The Open Cluster M35

289 citations · 5k across the 82 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.SR2012★ 44 cited

A Long-Period Totally Eclipsing Binary Star at the Turnoff of the Open Cluster NGC 6819 Discovered with Kepler

Eric L. Sandquist, Robert D. Mathieu, Karsten Brogaard +11

We present the discovery of the totally eclipsing long-period (P = 771.8 d) binary system WOCS 23009 in the old open cluster NGC 6819 that contains both an evolved star near centra…

astro-ph.SR2012★ 108 cited

Direct N-Body Modeling of the Old Open Cluster NGC 188: A Detailed Comparison of Theoretical and Observed Binary Star and Blue Straggler Populations

Aaron M. Geller, Jarrod R. Hurley, Robert D. Mathieu

(Abridged) Following on from a recently completed radial-velocity survey of the old (7 Gyr) open cluster NGC 188 in which we study in detail the solar-type hard binaries and blue s…

astro-ph.SR2012★ 181 cited

Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. age dependencies and new insights

K. Brogaard, D. A. VandenBerg, H. Bruntt +11

Models of stellar structure and evolution can be constrained by measuring accurate parameters of detached eclipsing binaries in open clusters. Multiple binary stars provide the mea…

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