A Subaru search for Lyα emitters at redshift 5.7

被引:99
作者
Ajiki, M [1 ]
Taniguchi, Y
Fujita, SS
Shioya, Y
Nagao, T
Murayama, T
Yamada, S
Umeda, K
Komiyama, Y
机构
[1] Tohoku Univ, Grad Sch Sci, Astron Inst, Aoba Ku, Sendai, Miyagi 9808578, Japan
[2] Natl Astron Observ Japan, Hilo, HI 96720 USA
关键词
cosmology : observations; early universe; galaxies : evolution; galaxies : formation;
D O I
10.1086/378481
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a survey for Lyalpha emitters at zapproximate to5.7 based on optical narrowband (lambda(c)=8150 Angstrom and Deltalambda=120 Angstrom) and broadband (B, R-C, I-C, and z') observations of the field surrounding the high-redshift quasar SDSSp J104433.04-012522.2 with the 8.2 m Subaru Telescope using the Subaru prime-focus camera, Suprime-Cam. This survey covers a sky area of approximate to720 arcmin(2) and a comoving volume of similar or equal to2x10(5) h(0.7)(-3) Mpc(3). We have found 20 candidate Lyalpha emitters at zapproximate to5.7 with Deltazapproximate to0.1. Two of them have been confirmed as star-forming galaxies at z=5.655 and z=5.687 from our follow-up optical spectroscopy. We discuss the star formation properties of the 20 objects from a statistical point of view. Our survey leads to a new estimate of the star formation rate density at zapproximate to5.7, similar to1.2x10(-3) h(0.7) M-circle dot yr(-1) Mpc(-3).
引用
收藏
页码:2091 / 2107
页数:17
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