2024-03-28T20:14:53Zhttp://digital.csic.es/dspace-oai/requestoai:digital.csic.es:10261/1406492018-06-25T08:48:31Zcom_10261_37com_10261_4col_10261_290
2016-11-23T12:10:56Z
urn:hdl:10261/140649
Planck intermediate results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories
Ade, P. A. R.
Aghanim, N.
Barreiro, R. Belén
Bernard, J. P.
Bouchet, F. R.
Bonavera, Laura
Curto, Andrés
Zotti, G. de
Diego, José María
González-Nuevo, J.
Herranz, D.
Hernández-Monteagudo, C.
Levrier, F.
López-Caniego, M.
Macías-Pérez, J. F.
Martínez-González, Enrique
Matarrese, S.
Rocha, G.
Rubiño-Martín, J. A.
Toffolatti, L.
Vielva, P.
Planck Collaboration
Ministerio de Economía y Competitividad (España)
European Space Agency
Centre National de la Recherche Scientifique (France)
Istituto Nazionale di Astrofisica
National Aeronautics and Space Administration (US)
Science and Technology Facilities Council (UK)
Academy of Finland
Center for Science (Finland)
Agenzia Spaziale Italiana
Department of Energy (US)
UK Space Agency
Fundação para a Ciência e a Tecnologia (Portugal)
Science Foundation Ireland
DTU Space (Denmark)
Swiss Space Office
Max Planck Society
German Centre for Air and Space Travel
European Commission
Consejo Superior de Investigaciones Científicas (España)
Junta de Andalucía
European Research Council
Large-scale structure of universe
Galaxies: clusters: general
Catalogues
Catalogs and data.-- et al.
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).
2016-11-23T12:10:56Z
2016-11-23T12:10:56Z
2016
2016-11-23T12:10:56Z
artículo
Astronomy and Astrophysics 586: A139 (2016)
http://hdl.handle.net/10261/140649
10.1051/0004-6361/201526345
http://dx.doi.org/10.13039/501100003329
http://dx.doi.org/10.13039/501100000844
http://dx.doi.org/10.13039/501100004794
http://dx.doi.org/10.13039/501100005184
http://dx.doi.org/10.13039/100000104
http://dx.doi.org/10.13039/501100000271
http://dx.doi.org/10.13039/501100003981
http://dx.doi.org/10.13039/501100001871
http://dx.doi.org/10.13039/501100001602
http://dx.doi.org/10.13039/501100004189
http://dx.doi.org/10.13039/501100002946
http://dx.doi.org/10.13039/501100000780
http://dx.doi.org/10.13039/501100003339
http://dx.doi.org/10.13039/501100000781
http://dx.doi.org/10.13039/501100002341
http://dx.doi.org/10.13039/100000015
http://dx.doi.org/10.13039/100011690
http://dx.doi.org/10.13039/501100011011
eng
Publisher's version
http://dx.doi.org/10.1051/0004-6361/201526345
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openAccess
EDP Sciences