Author ORCID Identifier
Document Type
Article
Publication Date
2-14-2017
Abstract
The Candidate Cluster and Protocluster Catalog contains 218 galaxy overdensities composed of more than 2000 galaxies with spectroscopic redshifts spanning the first few Gyr after the Big Bang (2.0 ≤ z < 6.6). We use Spitzer archival data to track the underlying stellar mass of these overdense regions in various temporal cross sections by building rest-frame near-infrared luminosity functions (LFs) across the span of redshifts. This exercise maps the stellar growth of protocluster galaxies, as halos in the densest environments should be the most massive from hierarchical accretion. The characteristic apparent magnitude, m∗(z), is relatively flat from 2.0 ≤ z < 6.6, consistent with a passive evolution of an old stellar population. This trend maps smoothly to lower redshift results of cluster galaxies from other works. We find no difference in the LFs of galaxies in the field versus protoclusters at a given redshift apart from their density.
Keywords
galaxies: clusters: general, galaxies: evolution, galaxies: high-redshift
Language
English
Publication Title
Astrophysical Journal
Grant
NAS5-26555
Rights
© The American Astronomical Society. All rights reserved. This content is free to access, download, and share. For all other uses, you must obtain permission to reuse content: https://journals.aas.org/article-charges-and-copyright/#AAS_material
Recommended Citation
J. R. Franck and S. S. McGaugh 2017. Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC). ApJ 836 136
Manuscript Version
Final Publisher Version