Probing dark energy with future redshift surveys: a comparison of emission line and broad-band selection in the near-infrared

Authors :: Yun Wang
Andrea Cimatti
Carlton M. Baugh
Cedric G. Lacey
Alvaro Orsi
G. Zamorani
Source :: Monthly Notices of the Royal Astronomical Society.
Publication Year :: 2010
Publisher :: Oxford University Press (OUP), 2010.
Abstract: Future galaxy surveys will map the galaxy distribution in the redshift interval $0.5 -15.4$; a flux limit of at least $\logfha = -16$ is required for an \ha sample to become competitive in effective volume.

Subjects :: Physics
Near-infrared spectroscopy
Flux
Broad band
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
Redshift
Galaxy
Space and Planetary Science
Dark energy
Emission spectrum
Astrophysics::Galaxy Astrophysics
Selection (genetic algorithm)

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