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Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories

  • P. A.R. Ade
  • , N. Aghanim
  • , M. Arnaud
  • , M. Ashdown
  • , J. Aumont
  • , C. Baccigalupi
  • , A. J. Banday
  • , R. B. Barreiro
  • , R. Barrena
  • , N. Bartolo
  • , E. Battaner
  • , K. Benabed
  • , A. Benoit-Lévy
  • , J. P. Bernard
  • , M. Bersanelli
  • , P. Bielewicz
  • , I. Bikmaev
  • , H. Böhringer
  • , A. Bonaldi
  • , L. Bonavera
  • J. R. Bond, J. Borrill, F. R. Bouchet, R. Burenin, C. Burigana, E. Calabrese, J. F. Cardoso, A. Catalano, A. Chamballu, R. R. Chary, H. C. Chiang, G. Chon, P. R. Christensen, D. L. Clements, L. P.L. Colombo, C. Combet, B. Comis, B. P. Crill, A. Curto, F. Cuttaia, H. Dahle, L. Danese, R. D. Davies, R. J. Davis, P. De Bernardis, A. De Rosa, G. De Zotti, J. Delabrouille, J. M. Diego, H. Dole, S. Donzelli, O. Doré, M. Douspis, X. Dupac, G. Efstathiou, F. Elsner, T. A. Enßlin, H. K. Eriksen, A. Ferragamo, F. Finelli, O. Forni, M. Frailis, A. A. Fraisse, E. Franceschi, S. Fromenteau, S. Galeotta, S. Galli, K. Ganga, R. T. Génova-Santos, M. Giard, E. Gjerløw, J. González-Nuevo, K. M. Górski, A. Gruppuso, F. K. Hansen, D. L. Harrison, A. Hempel, C. Hernández-Monteagudo, D. Herranz, S. R. Hildebrandt, E. Hivon, A. Hornstrup, W. Hovest, K. M. Huffenberger, G. Hurier, T. R. Jaffe, E. Keihänen, R. Keskitalo, I. Khamitov, T. S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, J. M. Lamarre, A. Lasenby, M. Lattanzi, C. R. Lawrence, R. Leonardi, J. León-Tavares, F. Levrier, H. Lietzen, M. Liguori, P. B. Lilje, M. Linden-Vørnle, M. López-Caniego, P. M. Lubin, J. F. Macías-Pérez, B. Maffei, D. Maino, N. Mandolesi, M. Maris, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, P. McGehee, A. Melchiorri, A. Mennella, M. Migliaccio, M. A. Miville-Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, P. Naselsky, F. Nati, P. Natoli, D. Novikov, I. Novikov, C. A. Oxborrow, L. Pagano, F. Pajot, D. Paoletti, F. Pasian, O. Perdereau, V. Pettorino, F. Piacentini, M. Piat, E. Pierpaoli, S. Plaszczynski, E. Pointecouteau, G. Polenta, G. W. Pratt, S. Prunet, J. L. Puget, J. P. Rachen, R. Rebolo, M. Reinecke, M. Remazeilles, C. Renault, A. Renzi, I. Ristorcelli, G. Rocha, C. Rosset, M. Rossetti, G. Roudier, J. A. Rubiño-Martín*, B. Rusholme, M. Sandri, D. Santos, M. Savelainen, G. Savini, D. Scott, V. Stolyarov, A. Streblyanska, R. Sudiwala, R. Sunyaev, A. S. Suur-Uski, J. F. Sygnet, J. A. Tauber, L. Terenzi, L. Toffolatti, M. Tomasi, D. Tramonte, M. Tristram, M. Tucci, L. Valenziano, J. Valiviita, B. Van Tent, P. Vielva, F. Villa, L. A. Wade, B. D. Wandelt, I. K. Wehus, D. Yvon, A. Zacchei, A. Zonca
*Corresponding author for this work
  • Cardiff University
  • Institut d'Astrophysique Spatiale
  • CEA Saclay (Commissariat À l'Energie Atomique et Aux Energies Alternatives)
  • University of Cambridge
  • International School for Advanced Studies
  • IRAP
  • Universidad de Cantabria
  • University of La Laguna
  • Instituto de Astrofísica de Canarias
  • University of Padua
  • National Institute for Nuclear Physics
  • University of Granada
  • CNRS (UMR 7095)
  • Sorbonne Université
  • University College London
  • University of Milan
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Polish Academy of Sciences
  • Tatarstan Academy of Sciences
  • Kazan Volga Region Federal University
  • Max Planck Institute for Extraterrestrial Physics
  • University of Manchester
  • University of Toronto
  • Lawrence Berkeley National Laboratory
  • University of California at Berkeley
  • Moscow Institute of Physics and Technology
  • RAS - Space Research Institute
  • University of Ferrara
  • University of Oxford
  • APC - AstroParticule et Cosmologie
  • Laboratoire Traitement et Communication de l'Information
  • LERMA - Laboratoire d'Études du Rayonnement et de la Matière en Astrophysique et Atmosphères
  • Université Grenoble Alpes
  • CEA/Saclay
  • California Institute of Technology
  • University of KwaZulu-Natal
  • Princeton University
  • University of Copenhagen
  • Imperial College London
  • University of Southern California
  • Jet Propulsion Laboratory, California Institute of Technology
  • University of Oslo
  • University of Rome La Sapienza
  • Astronomical Observatory of Padua
  • Institut universitaire de France
  • European Space Astronomy Centre
  • Max Planck Institute for Astrophysics
  • Osservatorio Astronomico di Trieste
  • The University of Chicago
  • University of Oviedo
  • University of Warsaw
  • Universidad Andrés Bello
  • Centro de Estudios de Física Del Cosmos de Aragón (CEFCA)
  • Technical University of Denmark
  • Florida State University
  • University of Helsinki
  • Akdeniz University
  • Atacama Large Millimeter/submillimeter Array
  • European Southern Observatory
  • African Institute for Mathematical Sciences
  • University of Geneva
  • CGEE
  • Aalto University
  • University of Turku
  • Instituto Nacional de Astrofisica Optica y Electronica
  • University of California at Santa Barbara
  • Maynooth University
  • Italian Space Agency
  • RAS - P.N. Lebedev Physics Institute
  • Université Paris-Sud
  • Heidelberg University 
  • Osservatorio Astronomico Roma
  • Radboud University Nijmegen
  • CSIC
  • University of Rome Tor Vergata
  • University of British Columbia
  • RAS - Special Astrophysical Observatory
  • ESTEC
  • eCampus University
  • Université Paris-Sud
  • University of Illinois at Urbana-Champaign

Research output: Contribution to journal › Article › peer-review

19 Citations (Scopus)

Abstract

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the general optical follow-up programme undertaken by the Planck Collaboration. In total, 78 SZ sources are discussed. Deep-imaging observations were obtained for most of these sources; spectroscopic observations in either in long-slit or multi-object modes were obtained for many. We effectively used 37.5 clear nights. We found optical counterparts for 73 of the 78 candidates. This sample includes 53 spectroscopic redshift determinations, 20 of them obtained with a multi-object spectroscopic mode. The sample contains new redshifts for 27 Planck clusters that were not included in the first Planck SZ source catalogue (PSZ1).

Original languageEnglish
Article numberA139
JournalAstronomy and Astrophysics
Volume586
DOIs
Publication statusPublished - 1 Feb 2016
Externally publishedYes

Keywords

  • Large-scale structure of Universe
  • catalogs
  • galaxies: clusters: general

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