4.3 Article

The deep optical imaging of the Extended Groth Strip

期刊

RESEARCH IN ASTRONOMY AND ASTROPHYSICS
卷 9, 期 10, 页码 1061-1077

出版社

NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
DOI: 10.1088/1674-4527/9/10/001

关键词

galaxies: high-redshift; galaxies: photometry; surveys

资金

  1. China Scholarship Council (CSC)
  2. Jiangsu Planned Projects for Postdoctoral Research Funds [0802031C]
  3. K.C. Wong Education Foundation, Hong Kong
  4. Grants-in-Aid for Scientific Research [18072005] Funding Source: KAKEN

向作者/读者索取更多资源

We present u',g' R optical images taken with the MMT/Megacam and the Subaru/Suprime telescopes of the Extended Groth Strip survey. The total survey covers an area of about similar to 1 degree(2), including four sub-fields and is optimized for the study of galaxies at z similar to 3. Our methods for photometric calibration in AB magnitudes, the limiting magnitude and the galaxy number count are described. A sample of 1642 photometrically selected candidate Lyman-Break Galaxies (LBGs) to an apparent R(AB) magnitude limit of 25.0 is presented. The average sky surface density of our LBG sample is similar to 1.0 arcmin(-2), slightly higher than the previous finding.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.3
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据