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THE EVOLUTION OF THE FAR-UV LUMINOSITY FUNCTION AND STAR FORMATION RATE DENSITY OF THE CHANDRA DEEP FIELD SOUTH FROM z = 0.2 TO 1.2 WITH SWIFT /UVOT (2015)

First Author: Hagen L

Attributed to: MSSL Consolidated Grant 2013-16 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/808/2/178

Publication URI: http://dx.doi.org/10.1088/0004-637x/808/2/178

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2