A. Da Silva

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G. Chon

University College London

M. López-Caniego

European Space Astronomy Centre

J. F. Macías–Pérez

Laboratoire de Physique Subatomique et de Cosmologie

H. Kurki‐Suonio

University of Helsinki

J. A. Rubiño-Martín

Instituto de Astrofísica de Canarias

D. Scott

University of British Columbia

E. Franceschi

Osservatorio di Astrofisica e Scienza dello Spazio

A. Gregorio

Trieste Astronomical Observatory

F. Atrio‐Barandela

Universidad de Salamanca

R. Rébolo

Universidad de La Laguna

Cooperative Institutions

Centre National de la Recherche Scientifique

336

Université Paris Cité

129

University College London

128

National Institute for Astrophysics

123

Université Paris-Saclay

100

Commissariat à l'Énergie Atomique et aux Énergies Alternatives

University of Copenhagen

Princeton University

CEA Paris-Saclay

Flatiron Health (United States)

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Planck 2013 results. XXIX. The Planck catalogueof Sunyaev-Zeldovich sources

P. A. R. Ade N. Aghanim C. Armitage-Caplan M. Arnaud M. Ashdown

We describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations. The catalogue contains 1227 entries, making it over six times the size of the Planck Early SZ (ESZ) sample and the largest SZ-selected catalogue to date. It contains 861 confirmed clusters, of which 178 have been confirmed as clusters, mostly through follow-up observations, and a further 683 are previously-known clusters. The remaining 366 have the status of cluster candidates, and we divide them into three classes according to the quality of evidence that they are likely to be true clusters. The Planck SZ catalogue is the deepest all-sky cluster catalogue, with redshifts up to about one, and spans the broadest cluster mass range from (0.1 to 1.6) × 1015 M⊙. Confirmation of cluster candidates through comparison with existing surveys or cluster catalogues is extensively described, as is the statistical characterization of the catalogue in terms of completeness and statistical reliability. The outputs of the validation process are provided as additional information. This gives, in particular, an ensemble of 813 cluster redshifts, and for all these Planck clusters we also include a mass estimated from a newly-proposed SZ-mass proxy. A refined measure of the SZ Compton parameter for the clusters with X-ray counter-parts is provided, as is an X-ray flux for all the Planck clusters not previously detected in X-ray surveys.

Planck energy

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Euclid. I. Overview of the Euclid mission

Y. Mellier J. A. Acevedo Barroso A. Achúcarro Jiřı́ Adámek R. Adam

10.48550/arxiv.2405.13491

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Citations (11)