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Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS

Manzoni, G.; Scodeggio, M.; Baugh, C.M.; Norberg, P.; De Lucia, G.; Fritz, A.; Haines, C.P.; Zamorani, G.; Gargiulo, A.; Guzzo, L.; Iovino, A.; Małek, K.; Pollo, A.; Siudek, M.; Vergani, D.

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Authors

G. Manzoni

M. Scodeggio

G. De Lucia

A. Fritz

C.P. Haines

G. Zamorani

A. Gargiulo

L. Guzzo

A. Iovino

K. Małek

A. Pollo

M. Siudek

D. Vergani



Abstract

We study the evolution of the colour-magnitude relation for galaxies in the VIMOS Public Extragalactic Redshift Survey (VIPERS) by introducing the concept of the bright edge, and use this to derive constraints on the quenching of star formation activity in galaxies over the redshift range 0.5

Citation

Manzoni, G., Scodeggio, M., Baugh, C., Norberg, P., De Lucia, G., Fritz, A., …Vergani, D. (2021). Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS. New Astronomy, 84, Article 101515. https://doi.org/10.1016/j.newast.2020.101515

Journal Article Type Article
Acceptance Date Oct 1, 2020
Online Publication Date Oct 2, 2020
Publication Date 2021-04
Deposit Date Jul 22, 2021
Publicly Available Date Mar 28, 2024
Journal New Astronomy
Print ISSN 1384-1076
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 84
Article Number 101515
DOI https://doi.org/10.1016/j.newast.2020.101515
Related Public URLs https://arxiv.org/abs/1911.02445

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