Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Univ of Tokyo
NAOJ
U Tokyo
Subaru Telescope
U. Tokyo
NAOJ, ESO
National Astronomical Observatory of Japan
IoA, Cambridge
University of Durham
National Astroinomical Observatory of Japan
Univ of Durham
NAO, Japan
University of Tokyo
Institute of Astronomy, Univ. of Tokyo
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
Department of Astronomy, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan.
Department of Astronomy, School of Science, The University of Tokyo
Rio de Janeiro F.U., Brazil
NOAJ
Physics Institute, Universidade Federal do Rio de Janeiro
NAO, Japan;
Subaru
University of Rio de Janeiro, Brazil
Department of Physics, University of Arizona, Tucson, and Universidade Federal do Rio de Janeiro, Instituto de Fisica, Rio de Janeiro, Brazil
DESY
Rio de Janeiro Federal Univ.
Rio de Janeiro Federal U.
Univ of Durham, UK
Centro Brazileiro de Pesquisas Fisicas, Rio de Janeiro, Brazil
University of Tokyo, Japan
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Brazil
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Instituto de Física-UFRJ, Cx. Postal 68528, 21945-970 RJ, Rio de Janeiro, Brazil
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro.
Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, GB, Brasil
National Astronomical Observatory of Japan, Japan
National Astronomical Observatory of Japan, Tokyo, Japan
Department of Astronomy, University of Tokyo
National Astronomical Observatory, Japan
13th International Conference on Elastic and Diffractive Scattering (Blois Workshop) - Moving Forward into the LHC Era
A Bayesian Classifier for Photometric Redshifts: Identification of high redshift clusters
A Deficit of Faint Red Galaxies in the Possible Large-Scale Structures around the RDCS J1252.9-2927 Cluster at z=1.24
A galaxy populations study of a radio-selected protocluster at z~3.1
A Huge Filamentary Structure at z=0.55 and Star Formation Histories of Galaxies at z<1
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