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researcher

V. Villar

95 papers hereh-index 4210.7k citations150 works total

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

author position
  • sole author1
  • first author9
  • middle author56
  • last author13

Across the 79 of 95 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE60
  • astro-ph.IM9
  • astro-ph.CO8
  • astro-ph.GA7
  • astro-ph.SR6
  • astro-ph3
same name
  • V. Villar — 37 papers, h 8
  • V. Villar — 4 papers, h 6
  • V. Villar — 2 papers, h 5
  • V. Villar — 1 paper, h 1

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
20042026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 9.1k across the 95 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2007★ 97 cited

The Halpha-based Star Formation Rate Density of the Universe at z=0.84

Víctor Villar, Jesús Gallego, Pablo G. Pérez-González +5

We present the results of an Halpha near-infrared narrow-band survey searching for star-forming galaxies at redshift z=0.84. This work is an extension of our previous narrow-band s…

astro-ph2007★ 614 cited

The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer

Pablo G. Perez-Gonzalez, George H. Rieke, Victor Villar +8

Using a sample of ~28,000 sources selected at 3.6-4.5 microns with Spitzer observations of the HDF-N, the CDF-S, and the Lockman Hole (surveyed area: ~664 arcmin^2), we study the e…

astro-ph2004★ 112 cited

C, S, Zn and Cu abundances in planet-harbouring stars

A. Ecuvillon, G. Israelian, N. C. Santos +3

We present a detailed and uniform study of C, S, Zn and Cu abundances in a large set of planet host stars, as well as in a homogeneous comparison sample of solar-type dwarfs with n…

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