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Title: Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters

Abstract

Multi-band photometric and multi-object spectroscopic surveys of merging galaxy clusters allow for the characterization of the distributions of constituent DM and galaxy populations, constraints on the dynamics of the merging subclusters, and an understanding of galaxy evolution of member galaxies. We introduce deep photometric observations from Subaru/SuprimeCam and a catalog of 4431 spectroscopic galaxies from Keck/DEIMOS observations of 29 merging galaxy clusters ranging in redshift from z = 0.07 to 0.55. The ensemble is compiled based on the presence of radio relics, which highlight cluster-scale collisionless shocks in the intracluster medium. Together with the spectroscopic and photometric information, the velocities, timescales, and geometries of the respective merging events may be tightly constrained. In this preliminary analysis, the velocity distributions of 28 of the 29 clusters are shown to be well fit by single Gaussians. This implies that radio-relic mergers largely occur transverse to the line of sight and/or near-apocenter. Here, we present our optical and spectroscopic surveys, preliminary results, and a discussion of the value of radio-relic mergers for developing accurate dynamical models of each system.

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3];  [4]; ORCiD logo [5];  [5]; ORCiD logo [6]; ORCiD logo [7]; ORCiD logo [8]; ORCiD logo [9];  [10]; ORCiD logo [5];  [11]; ORCiD logo [12]
  1. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Univ. of California, Davis, CA (United States)
  2. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  3. Univ. of California, Davis, CA (United States); Univ. of Lisbon (Portugal)
  4. Univ. of California, Davis, CA (United States); Yonsei Univ., Seoul (Korea, Republic of)
  5. Univ. of California, Davis, CA (United States)
  6. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Leiden Univ. (Netherlands)
  7. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  8. Leiden Univ. (Netherlands); Lancaster Univ. (United Kingdom)
  9. Leiden Univ. (Netherlands); Univ. of Hamburg (Germany)
  10. Univ. of Hamburg (Germany)
  11. Yonsei Univ., Seoul (Korea, Republic of)
  12. The Ohio State Univ., Columbus, OH (United States)
Publication Date:
Research Org.:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1545292
Grant/Contract Number:  
AC52-07NA27344
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal. Supplement Series (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal. Supplement Series (Online); Journal Volume: 240; Journal Issue: 2; Journal ID: ISSN 1538-4365
Publisher:
American Astronomical Society/IOP
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; galaxies: clusters: intracluster medium; galaxies: distances and redshifts; large-scale structure of universe

Citation Formats

Golovich, N., Dawson, W. A., Wittman, D. M., Jee, M. J., Benson, B., Lemaux, B. C., van Weeren, R. J., Andrade-Santos, F., Sobral, D., de Gasperin, F., Brüggen, M., Bradač, M., Finner, K., and Peter, A. Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters. United States: N. p., 2019. Web. doi:10.3847/1538-4365/aaf88b.
Golovich, N., Dawson, W. A., Wittman, D. M., Jee, M. J., Benson, B., Lemaux, B. C., van Weeren, R. J., Andrade-Santos, F., Sobral, D., de Gasperin, F., Brüggen, M., Bradač, M., Finner, K., & Peter, A. Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters. United States. https://doi.org/10.3847/1538-4365/aaf88b
Golovich, N., Dawson, W. A., Wittman, D. M., Jee, M. J., Benson, B., Lemaux, B. C., van Weeren, R. J., Andrade-Santos, F., Sobral, D., de Gasperin, F., Brüggen, M., Bradač, M., Finner, K., and Peter, A. Wed . "Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters". United States. https://doi.org/10.3847/1538-4365/aaf88b. https://www.osti.gov/servlets/purl/1545292.
@article{osti_1545292,
title = {Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters},
author = {Golovich, N. and Dawson, W. A. and Wittman, D. M. and Jee, M. J. and Benson, B. and Lemaux, B. C. and van Weeren, R. J. and Andrade-Santos, F. and Sobral, D. and de Gasperin, F. and Brüggen, M. and Bradač, M. and Finner, K. and Peter, A.},
abstractNote = {Multi-band photometric and multi-object spectroscopic surveys of merging galaxy clusters allow for the characterization of the distributions of constituent DM and galaxy populations, constraints on the dynamics of the merging subclusters, and an understanding of galaxy evolution of member galaxies. We introduce deep photometric observations from Subaru/SuprimeCam and a catalog of 4431 spectroscopic galaxies from Keck/DEIMOS observations of 29 merging galaxy clusters ranging in redshift from z = 0.07 to 0.55. The ensemble is compiled based on the presence of radio relics, which highlight cluster-scale collisionless shocks in the intracluster medium. Together with the spectroscopic and photometric information, the velocities, timescales, and geometries of the respective merging events may be tightly constrained. In this preliminary analysis, the velocity distributions of 28 of the 29 clusters are shown to be well fit by single Gaussians. This implies that radio-relic mergers largely occur transverse to the line of sight and/or near-apocenter. Here, we present our optical and spectroscopic surveys, preliminary results, and a discussion of the value of radio-relic mergers for developing accurate dynamical models of each system.},
doi = {10.3847/1538-4365/aaf88b},
journal = {The Astrophysical Journal. Supplement Series (Online)},
number = 2,
volume = 240,
place = {United States},
year = {Wed Feb 13 00:00:00 EST 2019},
month = {Wed Feb 13 00:00:00 EST 2019}
}

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text, January 2009


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text, January 2010


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text, January 2010


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text, January 2011


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text, January 2011


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text, January 2014


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Constraining the efficiency of cosmic ray acceleration by cluster shocks
text, January 2016


Testing cosmic-ray acceleration with radio relics: a high-resolution study using MHD and tracers
text, January 2016


The Case for Electron Re-Acceleration at Galaxy Cluster Shocks
text, January 2017


A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E0657-56
text, January 2001


Multiple merging events in Abell 521
text, January 2002


Magnetic Field in Clusters of Galaxies
text, January 2004


Second Data Release of the 6dF Galaxy Survey
text, January 2005


Internal dynamics of the radio-halo cluster A2744
text, January 2006


Galaxy Harassment and the Evolution of Clusters of Galaxies
text, January 1995


Bayesian photometric redshift estimation
text, January 1998


Works referencing / citing this record:

Polarization of radio relics in galaxy clusters
journal, November 2019

  • Wittor, D.; Hoeft, M.; Vazza, F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 3
  • DOI: 10.1093/mnras/stz2715

Brightest Cluster Galaxy Alignments in Merging Clusters
journal, March 2019

  • Wittman, David; Foote, Drake; Golovich, Nathan
  • The Astrophysical Journal, Vol. 874, Issue 1
  • DOI: 10.3847/1538-4357/ab0a0a

Multiwavelength Analysis of the Merging Galaxy Cluster A115
journal, April 2019


Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
journal, September 2019

  • Golovich, N.; Dawson, W. A.; Wittman, D. M.
  • The Astrophysical Journal, Vol. 882, Issue 1
  • DOI: 10.3847/1538-4357/ab2f90

Dynamical Properties of Merging Galaxy Clusters from Simulated Analogs
journal, August 2019


Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
text, January 2018


Brightest Cluster Galaxy Alignments in Merging Clusters
text, January 2018