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Clustering properties of 1.1 mm-selected submillimetre galaxies uncovered by AzTEC deep surveys

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Clustering properties of 1.1 mm-selected submillimetre galaxies uncovered by AzTEC deep surveys

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dc.contributor.author Hatsukade, B. pl
dc.contributor.author Takeuchi, T. T. pl
dc.contributor.author Pollo, Agnieszka [SAP11018773] pl
dc.contributor.author Kohno, K. pl
dc.contributor.author Aretxaga, I. pl
dc.contributor.author Austermann, J. E. pl
dc.contributor.author Ezawa, H. pl
dc.contributor.author Hughes, D. H. pl
dc.contributor.author Ikarashi, S. pl
dc.contributor.author Iono, D. pl
dc.contributor.author Kawabe, R. pl
dc.contributor.author Nakanishi, K. pl
dc.contributor.author Oshima, T. pl
dc.contributor.author Perera, T. pl
dc.contributor.author Scott, K. S. pl
dc.contributor.author Tamura, Y. pl
dc.contributor.author Williams, C. C. pl
dc.contributor.author Wilson, G. W. pl
dc.contributor.author Yun, M. S. pl
dc.contributor.editor Ryohei, Kawabe pl
dc.contributor.editor Nario, Kuno pl
dc.contributor.editor Satoshi, Yamamoto pl
dc.date.accessioned 2015-06-29T17:28:52Z
dc.date.available 2015-06-29T17:28:52Z
dc.date.issued 2013 pl
dc.identifier.isbn 978-1-58381-836-7 pl
dc.identifier.uri http://ruj.uj.edu.pl/xmlui/handle/item/10698
dc.language eng pl
dc.title Clustering properties of 1.1 mm-selected submillimetre galaxies uncovered by AzTEC deep surveys pl
dc.type BookSection pl
dc.pubinfo San Francisco : Astronomical Society of the Pacific pl
dc.description.physical 269-270 pl
dc.abstract.en We performed deep and wide-field surveys at 1.1 mm using AzTEC camera mounted on ASTE. We calculate the two-point angular autocorrelation functions in seven deep survey fields: AKARI Deep Field South (ADF-S), COSMOS, GOODS-N, GOODS-S, Lockman Hole East, SSA 22, and SXDF. We detect evidence for clustering signals in all the fields. By averaging the results on the bright sources measured in the ADF-S, the SSA 22, and the SXDF fields, we derived a more significant correlation function of 1.1 mm sources. A comparison of the correlation length with a bias evolution model of dark halos suggests that dark halos hosting bright 1.1 mm sources evolve into galaxy clusters in the present-day universe. pl
dc.description.series Astronomical Society of the Pacific Conference Series, ISSN 1050-3390; vol. 476 pl
dc.description.publication 0,2 pl
dc.description.conftype international pl
dc.identifier.eisbn 978-1-58381-837-4 pl
dc.title.container New Trends in Radio Astronomy in the ALMA Era : the 30th Anniversary of Nobeyama Radio Observatory, Hakone, Japan, December 3-8, 2012 pl
dc.language.container eng pl
dc.affiliation Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne pl
dc.subtype ConferenceProceedings pl
dc.conference New Trends in Radio Astronomy in the ALMA Era; 2012-12-03; 2012-12-08; Hakone; Japonia; indeksowana w Web of Science; ; ; pl
dc.rights.original bez licencji pl


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