Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ETH-Zurich
ETH Zurich
ETH Zuerich;
Department of Astrophysics, ETH Zurich
Institute of Astronomy, Department of Physics, ETH Zurich, Switzerland
ETHZ
Herzberg Institute
HIA
U. of Toronto
Princeton University, Princeton, NJ
Royal Observatory, Edinburgh, Scotland; Princeton University, New Observatory, Princeton, NJ
Kitt Peak National Observatory, Tucson, AZ; Princeton University, New Observatory, Princeton, NJ
Hawaii, University, Honolulu
Hawaii, University, Honolulu; Toronto, University, Canada
University of Toronto
Princeton University, New Observatory, NJ
Herzberg Institute for Astrophysics
Zürich
Edinburgh, University; Royal Observatory, Edinburgh, Scotland
Princeton University Observatory, NJ
ETH Zürich, Switzerland
ETH Zürich, Institute of Astronomy, Switzerland
Princeton University, New Observatory Princeton, NJ
ETH-Zürich
Department Astronomy, University of Toronto
Dominion Astrophysical Observatory, Victoria, BC, Canada
Department of Astronomy, University of Toronto
Institute for Astronomy, ETH Zürich, Wolfgang-Pauli-strasse 27, 8093 Zürich, Switzerland
Department of Astronomy and Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada; and Department of Physics, Swiss Federal Institute of Technology Zürich, ETH Zentrum CH-8092 Zürich, Switzerland
Toronto Univ., Canada
Toronto University
University of Toronto, Toronto, Ontario, Canada
Swiss Federal Institute of Technology, ETH Zürich, Switzerland
Swiss Federal Institute of Technology Zürich, Switzerland
15 Micron Infrared Space Observatory Observations of the 1415+52 Canada-France Redshift Survey Field: The Cosmic Star Formation Rate as Derived from Deep Ultraviolet, Optical, Mid-Infrared, and Radio Photometry
15um ISO observations of a CFRS field: the cosmic SFR as derived from UV, optical, mid-IR and radio photometry
A change in the cluster environments of radio galaxies with cosmic epoch
A cosmologically significant population of galaxies dominated by very young star formation
A deep band I-band selected galaxy sample - Implications for galaxy evolution
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Profile ID: LFWR-SCP-P-31515