Stellar mass function of cluster galaxies at z ~ 1.5: Evidence for reduced quenching efficiency at high redshift

Julie B. Nantais, Remco F.J. Van Der Burg, Chris Lidman, Ricardo Demarco, Allison Noble, Gillian Wilson, Adam Muzzin, Ryan Foltz, Andrew Degroot, Michael C. Cooper

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

60 Citas (Scopus)


We present the stellar mass functions (SMFs) of passive and star-forming galaxies with a limiting mass of 1010.1MȮ in four spectroscopically confirmed Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS) galaxy clusters at 1.37 <z< 1.63. The clusters have 113 spectroscopically confirmed members combined, with 8-45 confirmed members each. We construct Ks-band-selected photometric catalogs for each cluster with an average of 11 photometric bands ranging from u to 8 μm. We compare our cluster galaxies to a field sample derived from a similar Ks-band-selected catalog in the UltraVISTA/COSMOS field. The SMFs resemble those of the field, but with signs of environmental quenching. We find that 30 ± 20% of galaxies that would normally be forming stars in the field are quenched in the clusters. The environmental quenching efficiency shows little dependence on projected cluster-centric distance out to ~4 Mpc, providing tentative evidence of pre-processing and/or galactic conformity in this redshift range. We also compile the available data on environmental quenching efficiencies from the literature, and find that the quenching efficiency in clusters and in groups appears to decline with increasing redshift in a manner consistent with previous results and expectations based on halo mass growth.

Idioma originalInglés
Número de artículoA161
PublicaciónAstronomy and Astrophysics
EstadoPublicada - 1 ago. 2016

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial


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