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arXiv · 0911.0669

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

Alvaro Orsi·C. M. Baugh·C. G. Lacey·A. Cimatti·Y. Wang·G. Zamorani
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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.

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Alvaro Orsi, C. M. Baugh, C. G. Lacey, A. Cimatti, Y. Wang, G. Zamorani. 2009-11-03. Probing dark energy with future redshift surveys: A comparison of emission line and broad band selection in the near infrared. https://doi.org/10.1111/j.1365-2966.2010.16585.x

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