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Far-IR Galaxy Counts Expected in the Iris Survey

Published online by Cambridge University Press:  25 May 2016

T.T. Takeuchi ,
H. Hirashita ,
T. G. Hattori ,
K. Ohta  and
H. Shibai
T.T. Takeuchi
Affiliation:
Dept. of Astronomy, Kyoto Univ., Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-01, Japan
H. Hirashita
Affiliation:
Dept. of Astronomy, Kyoto Univ., Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-01, Japan
T. G. Hattori
Affiliation:
Dept. of Astronomy, Kyoto Univ., Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-01, Japan
K. Ohta
Affiliation:
Dept. of Astronomy, Kyoto Univ., Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-01, Japan
H. Shibai
Affiliation:
Division of Particle and Astrophysical Sciences, Nagoya Univ., Furo-cho, Chikusa-ku, Nagoya 464-01, Japan

Extract

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Infrared Imaging Surveyor (IRIS, officially Astro-F) is a satellite which will be launched in the winter of 2003. The main purpose of the IRIS mission is an all sky survey in the mid- and far-IR with a flux limit much deeper than that of IRAS. In order to examine the performance of the survey and to find a suitable set of bandpasses for tracing galaxy evolution and picking up protogalaxy candidates as effective as possible using IRIS, we estimated the FIR galaxy counts based on a simple model with various sets of cosmological parameters and evolution types.

Type
Deep Fields & Evolution
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 486
Copyright
Copyright © Kluwer 1999