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researcher

R. Barrena

4 papers here

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

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.CO1
  • astro-ph.GA1
ORCID 0000-0003-4969-232X
same name
  • R. Barrena — 54 papers, h 26
  • R. Barrena — 17 papers, h 14
  • R. Barrena — 4 papers, h 1
  • R. Barrena — 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
20022015
most citedPlanck 2013 results. I. Overview of products and scientific results

1.8k citations · 1.9k across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2015★ 23 cited

Fossil Group Origins VII. Galaxy substructures in fossil systems

S. Zarattini, M. Girardi, J. A. L. Aguerri +9

Fossil groups are expected to be the final product of galaxy merging within galaxy groups. In simulations, they are predicted to assemble their mass at high redshift. This early fo…

astro-ph.CO2013★ 1.8k cited

Planck 2013 results. I. Overview of products and scientific results

Planck Collaboration, P. A. R. Ade, N. Aghanim +398

The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sk…

astro-ph2003★ 40 cited

Optical and NIR Observations of the Afterglow of GRB 020813

S. Covino, D. Malesani, F. Tavecchio +28

We present optical and near-infrared (NIR) photometry of the bright afterglow of GRB 020813. Our data span from 3 hours to 4 days after the GRB event. A rather sharp achromatic bre…

astro-ph2002★ 114 cited

The Dynamical Status of the Cluster of Galaxies 1E0657-56

R. Barrena, A. Biviano, M. Ramella +2

We present the results of a new spectroscopic and photometric survey of the hot X-ray cluster 1E0657-56, at z=0.296. We determine the presence of a low velocity dispersion subclust…

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