Skip to main content
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.
Published Web Location
https://arxiv.org/pdf/1710.03230v1.pdfNo data is associated with this publication.
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
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.