Probing dark energy with future redshift surveys : a comparison of emission line and broad-band selection in the near-infrared.
- Orsi, A.
- Baugh, C.M.
- Lacey, C.G.
- Cimatti, A.
- Wang, Y.
- Zamorani, G.
Publication date
June 2010
DOI Publisher
Wiley ISSN
0035-8711 Journal
Monthly Notices of the Royal Astronomical Society Language
English Citation count (estimate)
46Abstract
Future galaxy surveys will map the galaxy distribution in the redshift interval 0.5 −15.4 and a flux limit of at least log(FHα[erg s−1 cm−2]) =−16 is required for an Hα sample to become competitive in effective volume
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