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researcher

V. Casanova

20 papers hereh-index 17785 citations54 works total

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

author position
  • middle author12
  • last author1

Across the 13 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP10
  • astro-ph.HE4
  • astro-ph3
  • astro-ph.SR3
same name
  • V. Casanova — 29 papers, h 9
  • V. Casanova — 3 papers, h 11
  • V. Casanova — 2 papers, h 2
  • V. Casanova — 2 papers, h 2
  • V. Casanova — 1 paper

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
20052026
most citedA giant exoplanet orbiting a very low-mass star challenges planet formation models

130 citations · 582 across the 20 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2018★ 27 cited

Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle

B. Toledo-Padrón, J. I. González Hernández, C. Rodríguez-López +58

The search for Earth-like planets around late-type stars using ultra-stable spectrographs requires a very precise characterization of the stellar activity and the magnetic cycle of…

astro-ph.SR2010★ 14 cited

The field high-amplitude SX Phe variable BL Cam: results from a multisite photometric campaign. II. Evidence of a binary - possibly triple - system

S. Fauvaud, J. -P. Sareyan, I. Ribas +45

Short-period high-amplitude pulsating stars of Population I (δ Sct stars) and II (SX Phe variables) exist in the lower part of the classical (Cepheid) instability strip. Most of…

astro-ph.SR2009★ 14 cited

HD172189: another step in furnishing one of the best laboratories known for asteroseismic studies

O. L. Creevey, K. Uytterhoeven, S. Martín-Ruiz +25

HD172189 is a spectroscopic eclipsing binary system with a rapidly-rotating pulsating delta Scuti component. It is also a member of the open cluster IC4756. These combined characte…

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