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institution

University of Nottingham

United Kingdom

2.2k papers here114.4k citations across 2.2k
fields
  • astro-ph.GA374
  • quant-ph231
  • astro-ph170
  • astro-ph.CO168
  • gr-qc161
  • cond-mat.stat-mech112
  • hep-th110
  • cond-mat.mes-hall83
ROR 01ee9ar58OpenAlex

affiliations via OpenAlex

output
20022026
most citedDynamics of dark energy

6.3k citations

researchers with a paper here
  • C. Conselice153 · h 111
  • I. Lesanovsky65 · h 46
  • J. Carretero52 · h 74
  • R. Ivison50 · h 121
  • J. P. Garrahan49 · h 56
  • W. Hartley48 · h 74
  • O. Almaini47 · h 60
  • Weibin Li45 · h 29
  • F. Carollo44 · h 27
  • J. García-Bellido2 profiles43 · h 78
  • G. Tarlé41 · h 92
  • R. Miquel41 · h 88
collaborating institutions
  • Centre National de la Recherche ScientifiqueFR254 papers
  • University of CambridgeGB212 papers
  • University of EdinburghGB188 papers
  • University of OxfordGB168 papers
  • Royal ObservatoryGB167 papers
  • European Southern ObservatoryCL137 papers
  • University of ManchesterGB137 papers
  • University of PortsmouthGB137 papers
  • University College LondonGB131 papers
  • Leiden UniversityNL124 papers
  • Sorbonne UniversitéFR124 papers
  • Durham UniversityGB123 papers
Showing 2002 · astro-phShow all

2 papers · 2 filters

astro-ph2002

Star Formation Rate estimators: [OII]3727 vs. Halpha for local star-forming galaxies

A. Aragon-Salamanca, A. Alonso-Herrero, J. Gallego +4

The [OII]3727 emission line is frequently used as an indicator of the star formation rate (SFR) despite its complex dependence on metallicity and excitation conditions. We have ana…

astro-ph2002★ 8 cited

The Wave Mechanics of Large-scale Structure

Peter Coles

I review the basic ``gravitational instability'' model for the growth of structure in the expanding Universe. This model requires the existence of small initial irregularities in t…

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