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researcher

S. Andreon

393 papers hereh-index 386.3k citations516 works total

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

author position
  • sole author27
  • first author44
  • middle author94
  • last author13

Across the 178 of 393 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO173
  • astro-ph.GA112
  • astro-ph66
  • astro-ph.IM29
  • astro-ph.SR5
  • astro-ph.HE3
same name
  • S. Andreon — 12 papers

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
19942026
most citedSpectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey

877 citations · 7.2k across the 375 of their papers we have counts for

collaborators
Showing 2004Show all

4 papers · 1 filter

astro-ph2004★ 69 cited

Constraining dark energy models using the lookback time to galaxy clusters and the age of the universe

S. Capozziello, V. F. Cardone, M. Funaro +1

An impressive amount of different astrophysical data converges towards the picture of a spatially flat universe undergoing a today phase of accelerated expansion. The nature of the…

astro-ph2004★ 38 cited

Galaxy evolution in clusters up to z=1.0

S. Andreon, J. Willis, H. Quintana +3

We present a combined study of the colour-magnitude relation, colour distribution and luminosity function of a sample of 24 clusters at redshifts 0.3<z<1. The sample is largely com…

astro-ph2004★ 1 cited

Colour-detected clusters in the XMM Large Scale Structure Survey

S. Andreon, J. Willis, H. Quintana +3

We present first results on the use of a colour space filter for detecting galaxy clusters at cosmological redshifts in the XMM Large Scale Structure Survey. All clusters studied,…

astro-ph2004★ 1 cited

Galaxy evolution in clusters from z=1 to z=0

S. Andreon, J. Willis, H. Quintana +3

The XMM--LSS project is detecting distant clusters of low mass, quite comparable in mass to the ones in the local universe. This allows a direct comparison of galaxy properties at…

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