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R. Anderson

52 papers hereh-index 222.8k citations88 works total

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

author position
  • sole author10
  • first author11
  • middle author22
  • last author7

Across the 50 of 52 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR34
  • astro-ph.CO8
  • astro-ph.GA6
  • astro-ph.IM3
  • astro-ph.EP1
same name
  • R. Anderson — 39 papers, h 27
  • R. Anderson — 19 papers, h 14
  • R. Anderson — 14 papers, h 16
  • R. Anderson — 13 papers, h 17
  • R. Anderson — 10 papers, h 2
  • R. Anderson — 6 papers, h 17

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
20102023
most citedMilky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant

616 citations · 2.2k across the 52 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.SR2020★ 71 cited

The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations

Louise Breuval, Pierre Kervella, Richard I. Anderson +12

Classical Cepheids provide the foundation for the empirical extragalactic distance ladder. Milky Way Cepheids are the only stars in this class accessible to trigonometric parallax…

astro-ph.SR2020★ 2 cited

Towards precise and accurate Cepheid chemical abundances for 1% $\mbox{H}_0$ measurement: temperature determination

Sara Mancino, Martino Romaniello, Richard I. Anderson +1

One of the outstanding problems in modern physics is the origin is of accelerated expansion of the universe. High-precision determinations of the Hubble parameter $\mbox{H}_0$ at d…

astro-ph.SR2020

Cepheids under the magnifying glass -- not so simple, after all!

Richard I. Anderson

Classical Cepheids are blue loop stars that have famously been dubbed "magnifying glasses of stellar evolution" and have been studied for a long time. As more and more precise obse…

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