The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-αemitters fromz= 2 toz= 6

P. Cassata; L. Tasca; O. Le Fèvre; B. C. Lemaux; B. Garilli; V. Le Brun; D. Maccagni; L. Pentericci; R. Thomas; E. Vanzella; G. Zamorani; E. Zucca; R. Amorín; S. Bardelli; P. Capak; L. P. Cassará; M. Castellano; A. Cimatti; Jean-Gabriel Cuby; O. Cucciati; S. de la Torre; A. Durkalec; A. Fontana; Mauro Giavalisco; A. Grazian; Nimish P. Hathi; O. Ilbert; C. Moreau; S. Paltani; B. Ribeiro; M. Salvato; D. Schaerer; M. Scodeggio; V. Sommariva; M. Talia; Yoshiaki Taniguchi; L. Tresse; D. Vergani; P. W. Wang; S. Charlot; T. Contini; S. Fotopoulou; Anton M. Koekemoer; C. López-Sanjuán; Y. Mellier; N. Z. Scoville

doi:10.1051/0004-6361/201423824

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Abstract

Aims. The aim of this work is to constrain the evolution of the fraction of strong Lyα emitters among UV selected star-forming galaxies at 2 <z< 6, and to measure the stellar escape fraction of Lyα photons over the same redshift range.

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Cassata et al. (2014) studied this question.

synapsesocial.com/papers/6a7ecdf6e7861671be8eccfd https://doi.org/10.1051/0004-6361/201423824

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The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-αemitters fromz= 2 toz= 6

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The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-αemitters fromz= 2 toz= 6

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