학술논문
The miniJPAS survey: clusters and galaxy groups detection with AMICO
Document Type
Working Paper
Author
Maturi, M.; Finoguenov, A.; Lopes, P. A. A.; Delgado, R. M. González; Dupke, R. A.; Cypriano, E. S.; Carrasco, E. R.; Diego, J. M.; Penna-Lima, M.; Vílchez, J. M.; Moscardini, L.; Marra, V.; Bonoli, S.; Rodríguez-Martín, J. E.; Zitrin, A.; Márquez, I.; Hernán-Caballero, A.; Jiménez-Teja, Y.; Abramo, R.; Alcaniz, J.; Benitez, N.; Carneiro, S.; Cenarro, J.; Cristóbal-Hornillos, D.; Ederoclite, A.; López-Sanjuan, C.; Marín-Franch, A.; de Oliveira, C. Mendes; Moles, M.; Sodré Jr., L.; Taylor, K.; Varela, J.; Ramió, H. Vázquez; Fernández-Ontiveros, J. A.
Source
A&A 678, A145 (2023)
Subject
Language
Abstract
Samples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once their mass, position (for clustering studies) and redshift are known. In this context, large optical data sets play a crucial role. We investigate the capabilities of the Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) in detecting and characterizing galaxy groups and clusters. We analyze the data of the miniJPAS survey, obtained with the JPAS-Pathfinder camera and covering $1$ deg$^2$ centered on the AEGIS field to the same depths and with the same 54 narrow band plus 2 broader band near-UV and near-IR filters anticipated for the full J-PAS survey. We use the Adaptive Matched Identifier of Clustered Objects (AMICO) to detect and characterize groups and clusters of galaxies down to $S/N=2.5$ in the redshift range $0.05