Extreme-emission-line galaxies in the MUSE Hubble Ultra Deep Field Survey

Aims. We aim to apply a methodology to build a sample of extreme-emission-line galaxies (EELGs) using integral field spectroscopy data. In this work, we followed the spectroscopic criteria corresponding to EELG selection and used the MUSE Hubble Ultra-Deep Field Survey, which includes the deepest sp...

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Detalhes bibliográficos
Autores: del Moral-Castro, I., Vílchez Medina, José Manuel, Iglesias-Páramo, J., Arroyo-Polonio, A.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/369630
Acesso em linha:http://hdl.handle.net/10261/369630
Access Level:acceso abierto
Palavra-chave:Galaxies: evolution
Galaxies: starburst
Galaxies: star formation
Descrição
Resumo:Aims. We aim to apply a methodology to build a sample of extreme-emission-line galaxies (EELGs) using integral field spectroscopy data. In this work, we followed the spectroscopic criteria corresponding to EELG selection and used the MUSE Hubble Ultra-Deep Field Survey, which includes the deepest spectroscopic survey ever performed.

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