Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Oxford
U.C.Berkeley
UC Berkeley
Univ. of Oxford
NAPL, Oxford and Univ. of California, Berkeley
Oxford U.
IoA, Cambridge & Univ. of California, Berkeley
U.C. Berkeley
University of Oxford
Dept of Astrophysics, University of Oxford, UK
Department of Astrophysics, University of Oxford;
U.C.-Berkeley, IAP, IOA
Oxford Astrophysics
Dpt.Astron.&Phys., Univ.Calif., Berkeley, USA
University of California, Berkeley
UCB
Uni.Oxford, GB and IAP, Paris France
Astronomy Department and Center for Particle Astrophysics, University of California, Berkeley
Oxford University
Department of Physics and Astrophysics, 1 Keble Road, University of Oxford, OX1 3NP, UK; and Departments of Physics and Astronomy, University of California, Berkeley, CA 94720
California, University, Berkeley
University of Oxford, OX1 3RH, UK
Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 4LN, UK of Astronomy, University of California at Berkeley, Berkeley, CA 94720, USA
Harvard College Observatory, Smithsonian Astrophysical Observatory, Cambridge, Massachusetts.
Departments of Astronomy and Physics, and Center for Particle Astrophysics, University of California, Berkeley, CA 94720
University of California, Berkeley, California 94720, USA
Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK of California, Berkeley, CA, US
Nuclear and Astrophysics Laboratory, Keble Road, Oxford, OX1 3RH, England, UK
University of Oxford, Keble Road, Oxford OX1 3RH, United Kingdom
Physics Department, Denys Wilkinson Bldg, Keble Road, Oxford OX1 3RH, UK
Department of Astronomy, University of California, Berkeley, California 94720, USA
Departments of Astronomy and Physics, University of California, Berkeley, California 97420, USA
Department of physics, University of Oxford, Oxford OX1 3RH, UK.
Nuclear and Astrophysics Lab. 1 Keble Road
A backwards approach to the formation of disk galaxies I. Stellar and gas content
A Bayesian non-parametric method to detect clusters in Planck data
A bimodal model for the galaxy luminosity function
A coincidence of disturbed morphology and blue UV colour: minor-merger driven star formation in early-type galaxies at z~0.6
A compressed cloud in the VELA supernova remnant
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