THE DEEP2 REDSHIFT SURVEY: Lyα EMITTERS IN THE SPECTROSCOPIC DATABASE

被引:25
作者
Sawicki, Marcin [1 ,2 ]
Lemaux, Brian C. [2 ,3 ]
Guhathakurta, Puragra [2 ]
Kirby, Evan N. [2 ]
Konidaris, Nicholas P. [2 ]
Martin, Crystal L. [4 ]
Cooper, Michael C. [5 ]
Koo, David C. [2 ]
Newman, Jeffrey A. [6 ]
Weiner, Benjamin J. [5 ]
机构
[1] St Marys Univ, Dept Phys & Astron, Halifax, NS B3H 3C3, Canada
[2] Univ Calif Santa Cruz, Dept Phys & Astron, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
[3] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
[4] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[5] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[6] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
基金
加拿大自然科学与工程研究理事会;
关键词
galaxies: evolution; galaxies: formation; galaxies: high-redshift; techniques: spectroscopic;
D O I
10.1086/591779
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first results of a search for Ly alpha emitters (LAEs) in the DEEP2 spectroscopic database that uses a search technique that is different from but complementary to traditional narrowband imaging surveys. We have visually inspected similar to 20% of the available DEEP2 spectroscopic data and have found nine high-quality LAEs with clearly asymmetric line profiles and an additional 10 objects of lower quality, some of which may also be LAEs. Our survey is most sensitive to LAEs at z = 4.4-4.9 and that is indeed where all but one of our high-quality objects are found. We find the number density of our spectroscopically discovered LAEs to be consistent with those found in narrowband imaging searches. The combined, averaged spectrum of our nine high-quality objects is well fit by a two-component model, with a second, lower amplitude component redshifted by similar to 420 km s (1) with respect to the primary Ly alpha line, consistent with large-scale outflows from these objects. We conclude by discussing the advantages and future prospects of blank-sky spectroscopic surveys for high-z LAEs.
引用
收藏
页码:884 / 898
页数:15
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