UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?

M.~L.~L. Dantas; P.~R.~T. Coelho; R.~S. de Souza; T.~S. Gonçalves

doi:10.1093/mnras/stz3609

UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?

M.~L.~L. Dantas, P.~R.~T. Coelho, R.~S. de Souza, T.~S. Gonçalves

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	2996-3011
Number of pages	16
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
Volume	492
Issue number	2
DOIs	https://doi.org/10.1093/mnras/stz3609
Publication status	Published - 1 Feb 2020

Keywords

methods: statistical
galaxies: evolution
galaxies: general
galaxies: elliptical and lenticular
cD
galaxies: stellar content
ultraviolet: general
Astrophysics - Astrophysics of Galaxies

Access to Document

10.1093/mnras/stz3609

Cite this

@article{5665f39194c440ce8efe883dee03d144,

title = "UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?",

keywords = "methods: statistical, galaxies: evolution, galaxies: general, galaxies: elliptical and lenticular, cD, galaxies: stellar content, ultraviolet: general, Astrophysics - Astrophysics of Galaxies",

author = "M.~L.~L. Dantas and P.~R.~T. Coelho and {de Souza}, R.~S. and T.~S. Gon{\c c}alves",

year = "2020",

month = feb,

day = "1",

doi = "10.1093/mnras/stz3609",

language = "English",

volume = "492",

pages = "2996--3011",

journal = "Monthly Notices of the Royal Astronomical Society (MNRAS)",

issn = "0035-8711",