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researcher

R. Davies

148 papers hereh-index 7627k citations529 works total

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

author position
  • sole author1
  • first author1
  • middle author104
  • last author21

Across the 127 of 148 papers where every author was matched, so the position is known.

fields
  • astro-ph58
  • astro-ph.GA46
  • astro-ph.CO41
  • astro-ph.IM2
  • physics.ao-ph1
same name
  • R. Davies — 135 papers, h 70
  • R. Davies — 131 papers, h 55
  • R. Davies — 58 papers, h 34
  • R. Davies — 47 papers, h 28
  • R. Davies — 43 papers, h 27
  • R. Davies — 42 papers, h 34

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
19962022
most citedThe Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

1.1k citations · 17.3k across the 147 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019★ 27 cited

Molecular Gas Inflows and Outflows in Ultraluminous Infrared Galaxies at z∼0.2 and one QSO at z=6.1

R. Herrera-Camus, E. Sturm, J. Graciá-Carpio +12

Aims. We aim to search and characterize inflows and outflows of molecular gas in four ultraluminous infrared galaxies (ULIRGs) at z∼0.2−0.3 and one distant QSO at z=6.13. Me…

astro-ph.GA2019★ 44 cited

AGN feedback in a galaxy merger: Multi-phase, galaxy-scale outflows including a fast molecular gas blob ~6 kpc away from IRAS F08572+3915

R. Herrera-Camus, A. Janssen, E. Sturm +12

To understand the role that AGN feedback plays in galaxy evolution we need in-depth studies of the multi-phase structure and energetics of galaxy-wide outflows. In this work we pre…

astro-ph.GA2019★ 10 cited

Unravelling the Origin of the Counter-Rotating Core in IC 1459 with KMOS and MUSE

Laura J. Prichard, Sam P. Vaughan, Roger L. Davies

The massive early-type galaxy (ETG) IC 1459 is a slowly rotating galaxy that exhibits a rapidly counter-rotating kinematically decoupled core (KDC, $R_{\rm KDC}\approx 5^{\prime\pr…

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