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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 2022Show all

3 papers · 1 filter

astro-ph.SR2022★ 11 cited

Discovery of a binary-origin classical Cepheid in a binary system with a 59-day orbital period

Bogumił Pilecki, Ian B. Thompson, Felipe Espinoza-Arancibia +8

We report the discovery of a surprising binary configuration of the double-mode Cepheid OGLE-LMC-CEP-1347 pulsating in the first (P_1=0.690d) and second overtone (P_2=0.556d) modes…

astro-ph.CO2022★ 37 cited

Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Elcio Abdalla, Guillermo Franco Abellán, Amin Aboubrahim +200

In this paper we will list a few important goals that need to be addressed in the next decade, also taking into account the current discordances between the different cosmological…

astro-ph.GA2022★ 36 cited

Do the majority of stars form as gravitationally unbound?

František Dinnbier, Pavel Kroupa, Richard I. Anderson

Some of the youngest stars (age ≲10 Myr) are clustered, while many others are observed scattered throughout star forming regions or in complete isolation. It has been int…

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