Properties of LBGs with [OIII] detection at z ∼ 3.5: The importance of including nebular emission data in SED fitting
Astronomy and astrophysics (Berlin), 2019-11, Vol.631, p.A123 [Peer Reviewed Journal]ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201935975
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