Target Selection and Validation of DESI Emission Line Galaxies
Résumé
The Dark Energy Spectroscopic Instrument (DESI) will precisely constrain cosmic expansion and the growth of structure by collecting $\sim$40 million extra-galactic redshifts across $\sim$80% of cosmic history and one third of the sky. The Emission Line Galaxy (ELG) sample, which will comprise about one-third of all DESI tracers, will be used to probe the Universe over the $0.6 < z < 1.6$ range, which includes the $1.1
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Astrophysique [astro-ph]INSPIRE HEP : Connectez-vous pour contacter le contributeur
https://hal.science/hal-03765885
Soumis le : mercredi 31 août 2022-15:42:55
Dernière modification le : mercredi 15 mai 2024-13:00:22
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Identifiants
- HAL Id : hal-03765885 , version 1
- ARXIV : 2208.08513
- DOI : 10.3847/1538-3881/acb213
- INSPIRE : 2138935
Citer
A. Raichoor, J. Moustakas, Jeffrey A. Newman, T. Karim, S. Ahlen, et al.. Target Selection and Validation of DESI Emission Line Galaxies. Astron.J., 2023, 165 (3), pp.126. ⟨10.3847/1538-3881/acb213⟩. ⟨hal-03765885⟩
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