Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Sussex
Imperial College, UK
Univ. Sussex
The XCS Collaboration
University of Sussex
Glasgow, University, Scotland; Sussex, University, Brighton, England
Astronomy Centre, University of Sussex, Falmer, Brighton BN1 9QH, UK
CFMC / INIC, Av. Prof. Gama Pinto, 2, P-1699 Lisbon-Codex, Portugal
Sussex Univ., Brighton, England
CFMC / INIC, Av. Prof. Gama Pinto 2, 1699 Lisboa Codex, Portugal
Astronomy Centre, Division of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
Astronomy Centre, University of Sussex, Brighton BN1 9QJ, United Kingdom
Division of Physics and Astronomy, University of Sussex, Brighton BN1 9QH United Kingdom
Division of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, United Kingdom
Division of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom
Sussex, University, Brighton, England
CFMC / INIC, Av. Prof. Gama Pinto 2, P-1699 Lisbon Cedex, Portugal
School of Mathematical and Physical Sciences, University of Sussex, Brighton BN1 9QH, United Kingdom
Astrophysics Group, Imperial College, Blackett Laboratory, Prince Consort Road, London SW7 2BZ, England, UK; Astronomy Centre, University of Sussex, Brighton BN1 9QJ, England, UK.
Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK
Astronomy Centre, Division of Physics and Astronomy, University of Sussex, Brighton BN1||9QH, United Kingdom
Division of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, UK
Astrophysics Group, Blackett Laboratory, Imperial College, London, SW7 2BZ, UK
Department of Physics and Astronomy, University of Glasgow, Glosgow G12 8QQ, UK
Department of Phys. & Astron., Glasgow Univ., UK
IC
A classification of scalar field potentials with cosmological scaling solutions
A dark energy view of inflation
A Massive Galaxy Cluster At z=1.45 From The XMM Cluster Survey: Discovery, Confirmation And Implications For The L-T Relation And Cosmology
A Nested Sampling Algorithm for Cosmological Model Selection
A new approach to the evolution of cosmological perturbations on large scales
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Profile ID: LFWR-SCP-P-6810