The HectoMAP Cluster Survey. I. redMaPPer Clusters
Abstract
We use the dense HectoMAP redshift survey to explore the properties of 104 redMaPPer cluster candidates. The redMaPPer systems in HectoMAP cover the full range of richness and redshift (0.08 < z < 0.60). Fifteen of the systems included in the Subaru/Hyper Suprime-Cam public data release are bona fide clusters. The median number of spectroscopic members per cluster is ~20. We include redshifts of 3547 member candidates listed in the redMaPPer catalog whether they are cluster members or not. Here, we evaluate the redMaPPer membership probability spectroscopically. The purity (number of real systems) in redMaPPer exceeds 90% even at the lowest richness. Three massive galaxy clusters (M ~ 2 × 1013 M ⊙) associated with X-ray emission in the HectoMAP region are not included in the public redMaPPer catalog with λrich > 20, because they lie outside the cuts for this catalog.
- Authors:
-
- Smithsonian Astrophysical Observatory, Cambridge, MA (United States)
- Western Washington Univ., Bellingham, WA (United States). Dept. of Physics and Astronomy
- Korea Inst. for Advanced Study, Seoul (Korea, Republic of). Quantum Universe Center
- SLAC National Accelerator Lab., Menlo Park, CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology
- Univ. di Torino, Torino (Italy). Dipt. di Fisica
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1436083
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 856; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; galaxies: clusters: general; large-scale structure of universe
Citation Formats
Sohn, Jubee, Geller, Margaret J., Rines, Kenneth J., Hwang, Ho Seong, Utsumi, Yousuke, and Diaferio, Antonaldo. The HectoMAP Cluster Survey. I. redMaPPer Clusters. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aab20b.
Sohn, Jubee, Geller, Margaret J., Rines, Kenneth J., Hwang, Ho Seong, Utsumi, Yousuke, & Diaferio, Antonaldo. The HectoMAP Cluster Survey. I. redMaPPer Clusters. United States. https://doi.org/10.3847/1538-4357/aab20b
Sohn, Jubee, Geller, Margaret J., Rines, Kenneth J., Hwang, Ho Seong, Utsumi, Yousuke, and Diaferio, Antonaldo. Thu .
"The HectoMAP Cluster Survey. I. redMaPPer Clusters". United States. https://doi.org/10.3847/1538-4357/aab20b. https://www.osti.gov/servlets/purl/1436083.
@article{osti_1436083,
title = {The HectoMAP Cluster Survey. I. redMaPPer Clusters},
author = {Sohn, Jubee and Geller, Margaret J. and Rines, Kenneth J. and Hwang, Ho Seong and Utsumi, Yousuke and Diaferio, Antonaldo},
abstractNote = {We use the dense HectoMAP redshift survey to explore the properties of 104 redMaPPer cluster candidates. The redMaPPer systems in HectoMAP cover the full range of richness and redshift (0.08 < z < 0.60). Fifteen of the systems included in the Subaru/Hyper Suprime-Cam public data release are bona fide clusters. The median number of spectroscopic members per cluster is ~20. We include redshifts of 3547 member candidates listed in the redMaPPer catalog whether they are cluster members or not. Here, we evaluate the redMaPPer membership probability spectroscopically. The purity (number of real systems) in redMaPPer exceeds 90% even at the lowest richness. Three massive galaxy clusters (M ~ 2 × 1013 M ⊙) associated with X-ray emission in the HectoMAP region are not included in the public redMaPPer catalog with λrich > 20, because they lie outside the cuts for this catalog.},
doi = {10.3847/1538-4357/aab20b},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 856,
place = {United States},
year = {Thu Apr 05 00:00:00 EDT 2018},
month = {Thu Apr 05 00:00:00 EDT 2018}
}
Web of Science
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