Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint

Abstract We present optical properties of the 26 most massive galaxy clusters in the South Pole Telescope 2500 sq-deg footprint. We find a general consistency between our results and results found in the literature on samples built with different selection techniques. Most interesting, we find a pre...

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Published in:Proceedings of the International Astronomical Union
Main Author: Zenteno, Alfredo
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2014
Subjects:
Online Access:http://dx.doi.org/10.1017/s1743921314010461
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921314010461
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spelling crcambridgeupr:10.1017/s1743921314010461 2023-05-15T18:22:02+02:00 Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint Zenteno, Alfredo 2014 http://dx.doi.org/10.1017/s1743921314010461 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921314010461 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Proceedings of the International Astronomical Union volume 10, issue S309, page 355-355 ISSN 1743-9213 1743-9221 Astronomy and Astrophysics Space and Planetary Science journal-article 2014 crcambridgeupr https://doi.org/10.1017/s1743921314010461 2022-04-07T08:00:22Z Abstract We present optical properties of the 26 most massive galaxy clusters in the South Pole Telescope 2500 sq-deg footprint. We find a general consistency between our results and results found in the literature on samples built with different selection techniques. Most interesting, we find a preference for an evolution in the slope of the Schechter function, α, with its value increasing at higher redshift. Article in Journal/Newspaper South pole Cambridge University Press (via Crossref) South Pole Proceedings of the International Astronomical Union 10 S309 355 355
institution Open Polar
collection Cambridge University Press (via Crossref)
op_collection_id crcambridgeupr
language English
topic Astronomy and Astrophysics
Space and Planetary Science
spellingShingle Astronomy and Astrophysics
Space and Planetary Science
Zenteno, Alfredo
Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
topic_facet Astronomy and Astrophysics
Space and Planetary Science
description Abstract We present optical properties of the 26 most massive galaxy clusters in the South Pole Telescope 2500 sq-deg footprint. We find a general consistency between our results and results found in the literature on samples built with different selection techniques. Most interesting, we find a preference for an evolution in the slope of the Schechter function, α, with its value increasing at higher redshift.
format Article in Journal/Newspaper
author Zenteno, Alfredo
author_facet Zenteno, Alfredo
author_sort Zenteno, Alfredo
title Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
title_short Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
title_full Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
title_fullStr Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
title_full_unstemmed Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint
title_sort galaxy population study of the 26 most massive galaxy clusters within the spt footprint
publisher Cambridge University Press (CUP)
publishDate 2014
url http://dx.doi.org/10.1017/s1743921314010461
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921314010461
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Proceedings of the International Astronomical Union
volume 10, issue S309, page 355-355
ISSN 1743-9213 1743-9221
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s1743921314010461
container_title Proceedings of the International Astronomical Union
container_volume 10
container_issue S309
container_start_page 355
op_container_end_page 355
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