Skip to main navigation Skip to search Skip to main content

The atacama cosmology telescope: A catalog of >4000 Sunyaev–Zel’dovich galaxy clusters

  • M. Hilton
  • , C. Sifón
  • , S. Naess
  • , M. Madhavacheril
  • , M. Oguri
  • , E. Rozo
  • , E. Rykoff
  • , S. Adhikari
  • , M. Aguena
  • , S. Aiola
  • , S. Allam
  • , S. Amodeo
  • , A. Amon
  • , J. Annis
  • , B. Ansarinejad
  • , T. M.C. Abbott
  • , C. Aros-Bunster
  • , J. E. Austermann
  • , S. Avila
  • , D. Bacon
  • N. Battaglia, J. A. Beall, D. T. Becker, G. M. Bernstein, E. Bertin, T. Bhandarkar, S. Bhargava, J. R. Bond, D. Brooks, D. L. Burke, E. Calabrese, M. Carrasco Kind, J. Carretero, S. K. Choi, A. Choi, C. Conselice, L. N. Da Costa, M. Costanzi, D. Crichton, K. T. Crowley, R. Dünner, E. V. Denison, M. J. Devlin, S. R. Dicker, H. T. Diehl, J. P. Dietrich, P. Doel, S. M. Duff, A. J. Duivenvoorden, J. Dunkley, S. Everett, S. Ferraro, A. Ferté, B. Flaugher, J. Frieman, I. Ferrero, P. A. Gallardo, J. García-Bellido, E. Gaztanaga, P. Giles, J. E. Golec, M. B. Gralla, S. Grandis, D. Gruen, D. W. Gerdes, R. A. Gruendl, J. Gschwend, G. Gutierrez, D. Han, W. G. Hartley, M. Hasselfield, J. C. Hill, G. C. Hilton, A. D. Hincks, S. R. Hinton, S. P.P. Ho, K. Honscheid, B. Hoyle, J. Hubmayr, K. M. Huffenberger, J. P. Hughes, A. T. Jaelani, B. Jain, D. J. James, T. Jeltema, S. Kent, K. Knowles, B. J. Koopman, K. Kuehn, O. Lahav, M. Lima, Y. T. Lin, M. Lokken, S. I. Loubser, N. MacCrann, M. A.G. Maia, T. A. Marriage, J. Martin, J. McMahon, P. Melchior, F. Menanteau, R. Miquel, K. Moodley, R. Morgan, T. Mroczkowski, F. Nati, L. B. Newburgh, M. D. Niemack, A. J. Nishizawa, H. Miyatake, R. L.C. Ogando, J. Orlowski-Scherer, L. A. Page, A. Palmese, B. Partridge, F. Paz-Chinchón, P. Phakathi, A. A. Plazas, N. C. Robertson, A. K. Romer, A. Carnero Rosell, E. Sanchez, E. Schaan, A. Schillaci, N. Sehgal, S. Serrano, T. Shin, S. M. Simon, M. Smith, M. Salatino, M. Soares-Santos, D. N. Spergel, S. T. Staggs, E. R. Storer, E. Suchyta, M. E.C. Swanson, G. Tarle, D. Thomas, C. To, H. Trac, J. N. Ullom, L. R. Vale, J. Van Lanen, E. M. Vavagiakis, J. De Vicente, R. D. Wilkinson, E. J. Wollack, Z. Xu, Y. Zhan
  • University of KwaZulu-Natal
  • Pontificia Universidad Católica de Valparaíso
  • Simons Foundation
  • Perimeter Institute for Theoretical Physics
  • The University of Tokyo
  • University of Arizona
  • Stanford University
  • SLAC National Accelerator Laboratory
  • Universidade de São Paulo
  • Laboratório Interinstitucional de e-Astronomia
  • Fermi National Accelerator Laboratory
  • Cornell University
  • Durham University
  • NSF's NOIRLab
  • National Institute of Standards and Technology
  • Universidad Autónoma de Madrid
  • University of Portsmouth
  • University of Pennsylvania
  • Institut d'Astrophysique de Paris
  • Sorbonne Université
  • University of Sussex
  • University of Toronto
  • University College London
  • Cardiff University
  • University of Illinois at Urbana-Champaign
  • Institute for High Energy Physics
  • Ohio State University
  • University of Manchester
  • University of Nottingham
  • Observatório Nacional
  • Osservatorio Astronomico di Trieste
  • University of Trieste
  • University of California at Berkeley
  • Pontificia Universidad Católica de Chile
  • Ludwig Maximilian University of Munich
  • Princeton University
  • University of California at Santa Cruz
  • Lawrence Berkeley National Laboratory
  • Jet Propulsion Laboratory, California Institute of Technology
  • The University of Chicago
  • University of Oslo
  • Institute of Space Studies of Catalonia
  • CSIC
  • University of Michigan, Ann Arbor
  • Stony Brook University
  • University of Geneva
  • Swiss Federal Institute of Technology Zurich
  • Columbia University
  • University of Queensland
  • Max Planck Institute for Extraterrestrial Physics
  • Florida State University
  • Rutgers - The State University of New Jersey, New Brunswick
  • Kindai University
  • Bandung Institute of Technology
  • Harvard-Smithsonian Ctr. Astrophys.
  • Yale University
  • Macquarie University
  • Lowell Observatory
  • Academia Sinica - Institute of Astronomy and Astrophysics
  • North West University
  • Johns Hopkins University
  • Half Hollow Hills High School East
  • ICREA
  • University of Wisconsin-Madison
  • European Southern Observatory
  • University of Milan - Bicocca
  • Nagoya University
  • Haverford College
  • University of Cambridge
  • Instituto de Astrofísica de Canarias
  • University of La Laguna
  • CIEMAT
  • California Institute of Technology
  • University of Southampton
  • Oak Ridge National Laboratory
  • Carnegie Mellon University
  • NASA Goddard Space Flight Center

Research output: Contribution to journalArticlepeer-review

134 Scopus citations

Abstract

We present a catalog of 4195 optically confirmed Sunyaev–Zel’dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio >4 in 13,211 deg2 of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multifrequency matched filter to 98 and 150 GHz maps constructed from ACT observations obtained from 2008 to 2018 and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z < 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ signal versus mass-scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M500c > 3.8 × 1014 Me, evaluated at z = 0.5, for clusters detected at signal-to-noise ratio >5 in maps filtered at an angular scale of 2 4. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ signal mass-scaling relation, such as the Dark Energy Survey (4566 deg2), the Hyper Suprime-Cam Subaru Strategic Program (469 deg2), and the Kilo Degree Survey (825 deg2). We highlight some noteworthy objects in the sample, including potentially projected systems, clusters with strong lensing features, clusters with active central galaxies or star formation, and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10 Gyr.

Original languageEnglish
Article numberabd023
JournalAstrophysical Journal, Supplement Series
Volume253
Issue number1
DOIs
StatePublished - Mar 2021

Fingerprint

Dive into the research topics of 'The atacama cosmology telescope: A catalog of >4000 Sunyaev–Zel’dovich galaxy clusters'. Together they form a unique fingerprint.

Cite this