中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5?

文献类型:期刊论文

作者Jiang,Linhua6; Shen,Yue4,5; Bian,Fuyan3; Zheng,Zhen-Ya1,2,15; Wu,Jin6,14; Oyarzún,Grecco A.12,13; Blanc,Guillermo A.11,13; Fan,Xiaohui9; Ho,Luis C.6,14; Infante,Leopoldo1
刊名The Astrophysical Journal
出版日期2017-09-11
卷号846期号:2
ISSN号0004-637X
关键词cosmology: observations galaxies: high-redshift galaxies: formation galaxies: evolution
DOI10.3847/1538-4357/aa8561
英文摘要Abstract We present a spectroscopic survey of high-redshift, luminous galaxies over four square degrees on the sky, aiming to build a large and homogeneous sample of Lyα emitters (LAEs) at z ≈ 5.7 and 6.5, and Lyman-break galaxies (LBGs) at 5.5 < z < 6.8 . The fields that we choose to observe are well studied, such as by the Subaru XMM-Newton Deep Survey and COSMOS. They have deep optical imaging data in a series of broad and narrow bands, allowing for the efficient selection of galaxy candidates. Spectroscopic observations are being carried out using the multi-object spectrograph M2FS on the Magellan Clay telescope. M2FS is efficient enough to identify high-redshift galaxies, owing to its 256 optical fibers deployed over a circular field of view 30 ′ in diameter. We have observed ~2.5 square degrees. When the program is completed, we expect to identify more than 400 bright LAEs at z ≈ 5.7 and 6.5, and a substantial number of LBGs at z ≥ 6 . This unique sample will be used to study a variety of galaxy properties and to search for large protoclusters. Furthermore, the statistical properties of these galaxies will be used to probe cosmic reionization. We describe the motivation, program design, target selection, and M2FS observations. We also outline our science goals, and present a sample of the brightest LAEs at z ≈ 5.7 and 6.5. This sample contains 32 LAEs with Lyα luminosities higher than 1043 erg s?1. A few of them reach ≥3?×?1043 erg s?1, comparable to the two most luminous LAEs known at z ≥ 6 , “CR7” and “COLA1.” These LAEs provide ideal targets to study extreme galaxies in the distant universe.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-846-2-AA8561
源URL[http://119.78.226.72/handle/331011/32103]  
专题中国科学院上海天文台
作者单位1.Institute of Astrophysics and Center for Astroengineering, Pontificia Universidad Catolica de Chile, Santiago 7820436, Chile
2.CAS Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Shanghai 200030, China
3.Research School of Astronomy and Astrophysics, Australian National University, Weston Creek, ACT 2611, Australia
4.National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA
5.Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA
6.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China ; jiangKIAA@pku.edu.cn
7.McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA
8.Leiden Observatory, Leiden University, P.O. Box 9513, 2300RA Leiden, The Netherlands
9.Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA
10.Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA
推荐引用方式
GB/T 7714
Jiang,Linhua,Shen,Yue,Bian,Fuyan,et al. A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5?
APA Jiang,Linhua.,Shen,Yue.,Bian,Fuyan.,Zheng,Zhen-Ya.,Wu,Jin.,...&Walker,Matthew G..(2017).A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5?The Astrophysical Journal,846(2).
MLA Jiang,Linhua,et al."A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5?The Astrophysical Journal 846.2(2017).

入库方式: OAI收割

来源:上海天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。