COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
Heidelberg University · Osservatorio astronomico di Bologna · +33 more institutions
Abstract
Aims. We investigate the redshift evolution and group richness dependence of the quiescent galaxy fraction and red sequence (RS) parameters in COSMOS galaxy groups, spanning a wide redshift range, from z = 0 to z = 3.7. Methods. We analyzed the deep and well-characterized sample of groups recently detected with the AMICO algorithm in the COSMOS(-Web) field. Our study of the quiescent galaxy population is based on a machine-learning classification tool based on rest-frame magnitudes. The algorithm learns from several traditional methods to estimate the probability of a galaxy being quiescent, achieving high precision and recall. Starting from this classification, we computed quiescent galaxy fractions within…
Citation impact
- FWCI
- 70.83
- Percentile
- 100%
- References
- 119
Authors
37- GTGreta ToniCorresponding
Heidelberg University, Osservatorio astronomico di Bologna, National Institute for Astrophysics
- MMM. Maturi
Heidelberg University
- GCG. Castignani
National Institute for Astrophysics
- LML. Moscardini
Osservatorio astronomico di Bologna, Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, National Institute for Astrophysics
- GGG. Gozaliasl
University of Helsinki, Aalto University
Topics & keywords
- Galaxy
- Interacting galaxy
- Brightest cluster galaxy
- Redshift
- Lenticular galaxy
- Population
- Galaxy group
- Galaxy formation and evolution