The evolution of the equivalent width of the Ha emission line and specific star-formation rate in star-forming galaxies at 1

Journal
Date Issued
2016
Author(s)
Marmol-Queralto, E.
•
McLure, R. J.
•
Cullen, F.
•
Dunlop, J. S.
•
•
McLeod, D. J.
DOI
Abstract
We present the results of a study which uses spectral energy distribution (SED) fitting to investigate the evolution of the equivalent width (EW) of the Halpha emission line in star-forming galaxies over the redshift interval 1=1 in the CANDELS UDS and GOODS-S fields. Confining our analysis to a constant stellar mass range (9.5
Volume
460
Issue
4
Start page
3587
Uri
Url
Issn Identifier
0035-8711
Ads BibCode
2016MNRAS.460.3587M
Rights
open.access
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