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

2013
book section
conference proceedings
Author
Hatsukade B.

Takeuchi T. T.

Pollo Agnieszka

Kohno K.

Aretxaga I.

Austermann J. E.

Ezawa H.

Hughes D. H.

Ikarashi S.

Iono D.

Kawabe R.

Nakanishi K.

Oshima T.

Perera T.

Scott K. S.

Tamura Y.

Williams C. C.

Wilson G. W.

Yun M. S.
Editor
Ryohei Kawabe

Nario Kuno

Satoshi Yamamoto
Book title / Journal title
New Trends in Radio Astronomy in the ALMA Era : the 30th Anniversary of Nobeyama Radio Observatory, Hakone, Japan, December 3-8, 2012
publisher
San Francisco : Astronomical Society of the Pacific
Pages
269-270
ISBN
978-1-58381-836-7
eISBN
978-1-58381-837-4
Series
Astronomical Society of the Pacific Conference Series
Serie's ISSN
1050-3390
Number of serie
vol. 476
Language
English
Book language / Journal language
English
Abstract in English

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.

Conference
New Trends in Radio Astronomy in the ALMA Era
Conference start date
2012-12-03
End date conference
2012-12-08
Conference city
Hakone
Conference country
Japonia
Conference type
Affiliation
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne
dc.abstract.enWe 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.affiliationWydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomicznepl
dc.conferenceNew Trends in Radio Astronomy in the ALMA Erapl
dc.conference.cityHakone
dc.conference.countryJaponia
dc.conference.datefinish2012-12-08
dc.conference.datestart2012-12-03
dc.conference.indexwostrue
dc.contributor.authorHatsukade, B.pl
dc.contributor.authorTakeuchi, T. T.pl
dc.contributor.authorPollo, Agnieszka - 131503 pl
dc.contributor.authorKohno, K.pl
dc.contributor.authorAretxaga, I.pl
dc.contributor.authorAustermann, J. E.pl
dc.contributor.authorEzawa, H.pl
dc.contributor.authorHughes, D. H.pl
dc.contributor.authorIkarashi, S.pl
dc.contributor.authorIono, D.pl
dc.contributor.authorKawabe, R.pl
dc.contributor.authorNakanishi, K.pl
dc.contributor.authorOshima, T.pl
dc.contributor.authorPerera, T.pl
dc.contributor.authorScott, K. S.pl
dc.contributor.authorTamura, Y.pl
dc.contributor.authorWilliams, C. C.pl
dc.contributor.authorWilson, G. W.pl
dc.contributor.authorYun, M. S.pl
dc.contributor.editorRyohei, Kawabepl
dc.contributor.editorNario, Kunopl
dc.contributor.editorSatoshi, Yamamotopl
dc.date.accessioned2015-06-29T17:28:52Z
dc.date.available2015-06-29T17:28:52Z
dc.date.issued2013pl
dc.description.conftypeinternationalpl
dc.description.physical269-270pl
dc.description.publication0,2pl
dc.description.seriesAstronomical Society of the Pacific Conference Series
dc.description.seriesnumbervol. 476
dc.identifier.eisbn978-1-58381-837-4pl
dc.identifier.isbn978-1-58381-836-7pl
dc.identifier.seriesissn1050-3390
dc.identifier.urihttp://ruj.uj.edu.pl/xmlui/handle/item/10698
dc.languageengpl
dc.language.containerengpl
dc.pubinfoSan Francisco : Astronomical Society of the Pacificpl
dc.rights.licencebez licencji
dc.subtypeConferenceProceedingspl
dc.titleClustering properties of 1.1 mm-selected submillimetre galaxies uncovered by AzTEC deep surveyspl
dc.title.containerNew Trends in Radio Astronomy in the ALMA Era : the 30th Anniversary of Nobeyama Radio Observatory, Hakone, Japan, December 3-8, 2012pl
dc.typeBookSectionpl
dspace.entity.typePublication
dc.abstract.enpl
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.
dc.affiliationpl
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne
dc.conferencepl
New Trends in Radio Astronomy in the ALMA Era
dc.conference.city
Hakone
dc.conference.country
Japonia
dc.conference.datefinish
2012-12-08
dc.conference.datestart
2012-12-03
dc.conference.indexwos
true
dc.contributor.authorpl
Hatsukade, B.
dc.contributor.authorpl
Takeuchi, T. T.
dc.contributor.authorpl
Pollo, Agnieszka - 131503
dc.contributor.authorpl
Kohno, K.
dc.contributor.authorpl
Aretxaga, I.
dc.contributor.authorpl
Austermann, J. E.
dc.contributor.authorpl
Ezawa, H.
dc.contributor.authorpl
Hughes, D. H.
dc.contributor.authorpl
Ikarashi, S.
dc.contributor.authorpl
Iono, D.
dc.contributor.authorpl
Kawabe, R.
dc.contributor.authorpl
Nakanishi, K.
dc.contributor.authorpl
Oshima, T.
dc.contributor.authorpl
Perera, T.
dc.contributor.authorpl
Scott, K. S.
dc.contributor.authorpl
Tamura, Y.
dc.contributor.authorpl
Williams, C. C.
dc.contributor.authorpl
Wilson, G. W.
dc.contributor.authorpl
Yun, M. S.
dc.contributor.editorpl
Ryohei, Kawabe
dc.contributor.editorpl
Nario, Kuno
dc.contributor.editorpl
Satoshi, Yamamoto
dc.date.accessioned
2015-06-29T17:28:52Z
dc.date.available
2015-06-29T17:28:52Z
dc.date.issuedpl
2013
dc.description.conftypepl
international
dc.description.physicalpl
269-270
dc.description.publicationpl
0,2
dc.description.series
Astronomical Society of the Pacific Conference Series
dc.description.seriesnumber
vol. 476
dc.identifier.eisbnpl
978-1-58381-837-4
dc.identifier.isbnpl
978-1-58381-836-7
dc.identifier.seriesissn
1050-3390
dc.identifier.uri
http://ruj.uj.edu.pl/xmlui/handle/item/10698
dc.languagepl
eng
dc.language.containerpl
eng
dc.pubinfopl
San Francisco : Astronomical Society of the Pacific
dc.rights.licence
bez licencji
dc.subtypepl
ConferenceProceedings
dc.titlepl
Clustering properties of 1.1 mm-selected submillimetre galaxies uncovered by AzTEC deep surveys
dc.title.containerpl
New Trends in Radio Astronomy in the ALMA Era : the 30th Anniversary of Nobeyama Radio Observatory, Hakone, Japan, December 3-8, 2012
dc.typepl
BookSection
dspace.entity.type
Publication
Affiliations
Wydział Fizyki, Astronomii i Informatyki Stosowanej
Pollo, Agnieszka
No affiliation
Hatsukade, B.
Takeuchi, T. T.
Kohno, K.
Aretxaga, I.
Austermann, J. E.
Ezawa, H.
Hughes, D. H.
Ikarashi, S.
Iono, D.
Kawabe, R.
Nakanishi, K.
Oshima, T.
Perera, T.
Scott, K. S.
Tamura, Y.
Williams, C. C.
Wilson, G. W.
Yun, M. S.
Ryohei, Kawabe
Nario, Kuno
Satoshi, Yamamoto

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