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.

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., Haines, C., Zamorani, G., Gargiulo, A., Guzzo, L., Iovino, A., Małek, K., Pollo, A., Siudek, M., & 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: Oct 2, 2022
• 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
• Public URL: https://durham-repository.worktribe.com/output/1245197
• Related Public URLs: https://arxiv.org/abs/1911.02445