학술논문
The MOSDEF Survey: Broad Emission Lines at z = 1.4–3.8* * Based on data obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, and was made possible by the generous financial support of the W. M. Keck Foundation.
Document Type
article
Author
Source
The Astrophysical Journal. 873(2)
Subject
Language
Abstract
We present results from the MOSFIRE Deep Evolution Field survey on broad flux from the nebular emission lines Hα, [N ii], [O iii], Hβ, and [S ii]. The sample consists of 127 star-forming galaxies at 1.37