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Subaru Suprime-Cam Weak Lensing Survey over 33 deg2

Published online by Cambridge University Press:  15 June 2005

Satoshi Miyazaki ,
T. Hamana ,
A. Refregier ,
R.J. Massey ,
R.S. Ellis  and
N. Kashikawa
Satoshi Miyazaki
Affiliation:
Subaru Telescope NAOJ, 650 N Aohoku Pl. Hilo HI 96720 USA
T. Hamana
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
A. Refregier
Affiliation:
Service d'Astrophysique CEA Saclay, Bat. 709 F-91191 Gif sur Yvette, France
R.J. Massey
Affiliation:
California Institute of Technology, 105-24 Astronomy, Pasadena CA 91125 USA
R.S. Ellis
Affiliation:
California Institute of Technology, 105-24 Astronomy, Pasadena CA 91125 USA
N. Kashikawa
Affiliation:
National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
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Abstract

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Under the currently popular CDM model, mass plays the major role in evolution of large scale structure of the universe. In order to examine the paradigm based on observations, it would be ideal to use purely mass selected object catalog. Weak lensing surveys enable a blind search of cluster scale objects, and thus could provide such catalogs. We are working on a weak lensing survey using Subaru Prime Focus Camera (Suprime-Cam). In this note, we introduce our survey strategy, and the status as well as the performance of Suprime-Cam as a weak lensing surveyor.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS225 , July 2004 , pp. 57 - 62
Copyright
© 2004 International Astronomical Union