The VIMOS Ultra Deep Survey: the reversal of the star-formation rate - density relation at 2 < z < 5

Lemaux, B.C.; Cucciati, O.; Le Fèvre, O.; Zamorani, G.; Lubin, L.M.; Hathi, N.; Ilbert, O.; Pelliccia, D.; Amorín, R.; Bardelli, S.; Cassata, P.; Gal, R.R.; Garilli, B.; Guaita, L.; Giavalisco, M.; Hung, D.; Koekemoer, A.; Maccagni, D.; Pentericci, L.; Leite Ribeiro, B.R.; Schaerer, D.; Shah, E.; Shen, L.; Staab, P.; Talia, M.; Thomas, R.; Tomczak, A.R.; Tresse, L.; Vanzella, E.; Vergani, D.; Zucca, E.

doi:10.1051/0004-6361/202039346

The VIMOS Ultra Deep Survey: the reversal of the star-formation rate - density relation at 2 < z < 5

Author(s):: Lemaux, B.C.; Cucciati, O.; Le Fèvre, O.; Zamorani, G.; Lubin, L.M.; Hathi, N.; Ilbert, O.; Pelliccia, D.; Amorín, R.; Bardelli, S.; Cassata, P.; Gal, R.R.; Garilli, B.; Guaita, L.; Giavalisco, M.; Hung, D.; Koekemoer, A.; Maccagni, D.; Pentericci, L.; Leite Ribeiro, B.R. (0000-0002-4844-0414); Schaerer, D.; Shah, E.; Shen, L.; Staab, P.; Talia, M.; Thomas, R.; Tomczak, A.R.; Tresse, L.; Vanzella, E.; Vergani, D.; Zucca, E.

Published: 2022
Publication type: Article / Letter to editor

Galaxies: EvolutionGalaxies: High-RedshiftGalaxies: Clusters: GeneralTechniques: PhotometricTechniques: SpectroscopicAstrophysics - Astrophysics of Galaxies

Date issued: 2022
Language: English
Is part of: Astronomy & Astrophysics (2022), A33
hdl: 1887/3561695
doi: 10.1051/0004-6361/202039346
URL: https://ui.adsabs.harvard.edu/abs/2022A&A...662A..33L

The VIMOS Ultra Deep Survey: the reversal of the star-formation rate - density relation at 2 < z < 5

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