학술논문
Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS)
Document Type
Working Paper
Author
Ruiz-Macias, Omar; Zarrouk, Pauline; Cole, Shaun; Norberg, Peder; Baugh, Carlton; Brooks, David; Dey, Arjun; Duan, Yutong; Eftekharzadeh, Sarah; Eisenstein, Daniel J.; Forero-Romero, Jaime E.; Gaztañaga, Enrique; Hahn, ChangHoon; Kehoe, Robert; Landriau, Martin; Lang, Dustin; Levi, Michael E.; Lucey, John; Meisner, Aaron M.; Moustakas, John; Myers, Adam D.; Palanque-Delabrouille, Nathalie; Poppett, Claire; Prada, Francisco; Raichoor, Anand; Schlegel, David J.; Schubnell, Michael; Tarlé, Gregory; Weinberg, David H.; Wilson, M. J.; Yèche, Christophe
Source
Res. Notes AAS 4 187 (2020)
Subject
Language
Abstract
The Dark Energy Spectroscopic Instrument (DESI) will execute a nearly magnitude-limited survey of low redshift galaxies ($0.05 \leq z \leq 0.4$, median $z \approx 0.2$). Clustering analyses of this Bright Galaxy Survey (BGS) will yield the most precise measurements to date of baryon acoustic oscillations and redshift-space distortions at low redshift. DESI BGS will comprise two target classes: (i) BRIGHT ($r<19.5$~mag), and (ii) FAINT ($19.5