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Simulations of Deep Optical and Near Infrared Extragalactic CountsMonte-Carlo simulations of three dimensional galaxy distributions are performed, following the prescription of Chokshi and Wright(1988), to study the photometric properties of evolving galaxy populations in the optical and near infrared bands to high redshifts.
Document ID
20060038859
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/35166
Authors
Chokshi, A.
Lonsdale, C.
Mazzei, P.
Zotti, G. De
Date Acquired
August 23, 2013
Publication Date
March 26, 1993
Publication Information
Publication: The Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
faint galaxies galaxy evolution

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