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E. Gaztañaga

4 papers hereh-index 41.8k citations6 works total

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-ph3
  • astro-ph.GA1
same name
  • E. Gaztañaga — 847 papers, h 91
  • E. Gaztañaga — 14 papers, h 2
  • E. Gaztañaga — 14 papers, h 13
  • E. Gaztañaga — 11 papers
  • E. Gaztañaga — 2 papers
  • E. Gaztañaga — 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
19932014
most citedLarge-Scale Structure of the Universe and Cosmological Perturbation Theory

1.9k citations · 2.3k across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2014★ 173 cited

An algorithm to build mock galaxy catalogues using MICE simulations

J. Carretero, F. J. Castander, E. Gaztanaga +2

We present a method to build mock galaxy catalogues starting from a halo catalogue that uses halo occupation distribution (HOD) recipes as well as the subhalo abundance matching (S…

astro-ph2001★ 1.9k cited

Large-Scale Structure of the Universe and Cosmological Perturbation Theory

F. Bernardeau, S. Colombi, E. Gaztanaga +1

We review the formalism and applications of non-linear perturbation theory (PT) to understanding the large-scale structure of the Universe. We first discuss the dynamics of gravita…

astro-ph1994★ 85 cited

Bias and high-order galaxy correlation functions in the APM Galaxy Survey

E. Gaztanaga, J. Frieman

On large scales, the higher order moments of the mass distribution, $S_J=\xibar_J/\xibar_2^{J-1}$, e.g., the skewness S3​ and kurtosis S4​, can be predicted using non-linear pe…

astro-ph1993★ 118 cited

High-order galaxy correlation functions in the APM Galaxy Survey

Enrique Gaztanaga

We estimate J-point galaxy averaged correlation functions $\wbar_J(θ)$ for J=2,...,9, in a sample of the APM Galaxy Survey with more than 1.3×106 galaxies and a depth $…

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