The evolution of the equivalent width of the Ha emission line and specific star-formation rate in star-forming galaxies at 1
Date Issued
2016
Author(s)
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
Issn Identifier
0035-8711
Ads BibCode
2016MNRAS.460.3587M
Rights
open.access
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