STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS
Kavli Institute for the Physics and Mathematics of the Universe · Carnegie Observatories · +5 more institutions
Abstract
We present Lya luminosity function (LF), clustering measurements, and Lya line profiles based on the largest sample, to date, of 207 Lya emitters (LAEs) at z=6.6 on the 1-deg^2 sky of Subaru/XMM-Newton Deep Survey (SXDS) field. Our z=6.6 Lya LF including cosmic variance estimates yields the best-fit Schechter parameters of phi*=8.5 +3.0/-2.2 x10^(-4) Mpc^(-3) and L*(Lya)=4.4 +/-0.6 x10^42 erg s^(-1) with a fixed alpha=-1.5, and indicates a decrease from z=5.7 at the >~90% confidence level. However, this decrease is not large, only =~30% in Lya luminosity, which is too small to be identified in the previous studies. A clustering signal of z=6.6 LAEs is detected for the first time. We obtain the correlation…
Citation impact
- FWCI
- 28.29
- Percentile
- 100%
- References
- 175
Authors
15- MOMasami OuchiCorresponding
Kavli Institute for the Physics and Mathematics of the Universe, Carnegie Observatories, The University of Tokyo
- KSKazuhiro Shimasaku
Tokyo University of Science, The University of Tokyo
- HFHisanori Furusawa
National Astronomical Observatory of Japan
- TSTomoki Saito
Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo
- MYMakiko Yoshida
The University of Tokyo
Topics & keywords
- Physics
- Reionization
- Astrophysics
- Redshift
- Luminosity
- Galaxy
- Halo
- Population