A strong clustering of FIR-selected galaxies in the AKARI All-Sky Survey

Tomoko Suzuki; Tsutomu T. Takeuchi; Agnieszka Pollo; Shinki Oyabu

doi:10.1017/S1743921314010382

A strong clustering of FIR-selected galaxies in the AKARI All-Sky Survey

Tomoko Suzuki, Tsutomu T. Takeuchi, Agnieszka Pollo, Shinki Oyabu

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

Abstract

Various previous galaxy surveys have revealed that different types of galaxies show different spatial distributions. By comparing their clustering strengths, we can investigate the relationship between the environments where galaxies reside and the properties of galaxies. This provides us vital information on when, where, and how galaxies are formed. In this study, we focus on FIR-selected galaxies from AKARI All-Sky Survey, which are considered to be dusty star-forming galaxies. We measure their power spectrum and compare our final result with previous studies using different galaxy samples detected at other wavelengths. It is found that there is the very clear wavelength dependence of the clustering strength.

Original language	English
Pages (from-to)	346-347
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	10
DOIs	https://doi.org/10.1017/S1743921314010382
Publication status	Published - 2014
Externally published	Yes

Keywords

Galaxies: evolution
Galaxies: formation
Galaxies: star formation
Infrared: galaxies

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

Access to Document

10.1017/S1743921314010382

Cite this

@article{c9d79221d88c41768bde52e0e35e5e08,

title = "A strong clustering of FIR-selected galaxies in the AKARI All-Sky Survey",

abstract = "Various previous galaxy surveys have revealed that different types of galaxies show different spatial distributions. By comparing their clustering strengths, we can investigate the relationship between the environments where galaxies reside and the properties of galaxies. This provides us vital information on when, where, and how galaxies are formed. In this study, we focus on FIR-selected galaxies from AKARI All-Sky Survey, which are considered to be dusty star-forming galaxies. We measure their power spectrum and compare our final result with previous studies using different galaxy samples detected at other wavelengths. It is found that there is the very clear wavelength dependence of the clustering strength.",

keywords = "Galaxies: evolution, Galaxies: formation, Galaxies: star formation, Infrared: galaxies",

author = "Tomoko Suzuki and Takeuchi, {Tsutomu T.} and Agnieszka Pollo and Shinki Oyabu",

note = "Publisher Copyright: {\textcopyright} International Astronomical Union 2015.",

year = "2014",

doi = "10.1017/S1743921314010382",

language = "English",

volume = "10",

pages = "346--347",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

TY - JOUR

T1 - A strong clustering of FIR-selected galaxies in the AKARI All-Sky Survey

AU - Suzuki, Tomoko

AU - Takeuchi, Tsutomu T.

AU - Pollo, Agnieszka

AU - Oyabu, Shinki

N1 - Publisher Copyright: © International Astronomical Union 2015.

PY - 2014

Y1 - 2014

N2 - Various previous galaxy surveys have revealed that different types of galaxies show different spatial distributions. By comparing their clustering strengths, we can investigate the relationship between the environments where galaxies reside and the properties of galaxies. This provides us vital information on when, where, and how galaxies are formed. In this study, we focus on FIR-selected galaxies from AKARI All-Sky Survey, which are considered to be dusty star-forming galaxies. We measure their power spectrum and compare our final result with previous studies using different galaxy samples detected at other wavelengths. It is found that there is the very clear wavelength dependence of the clustering strength.

AB - Various previous galaxy surveys have revealed that different types of galaxies show different spatial distributions. By comparing their clustering strengths, we can investigate the relationship between the environments where galaxies reside and the properties of galaxies. This provides us vital information on when, where, and how galaxies are formed. In this study, we focus on FIR-selected galaxies from AKARI All-Sky Survey, which are considered to be dusty star-forming galaxies. We measure their power spectrum and compare our final result with previous studies using different galaxy samples detected at other wavelengths. It is found that there is the very clear wavelength dependence of the clustering strength.

KW - Galaxies: evolution

KW - Galaxies: formation

KW - Galaxies: star formation

KW - Infrared: galaxies

UR - http://www.scopus.com/inward/record.url?scp=84922561304&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84922561304&partnerID=8YFLogxK

U2 - 10.1017/S1743921314010382

DO - 10.1017/S1743921314010382

M3 - Article

AN - SCOPUS:84922561304

VL - 10

SP - 346

EP - 347

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

A strong clustering of FIR-selected galaxies in the AKARI All-Sky Survey

Abstract

Keywords

ASJC Scopus subject areas

UN SDGs

Access to Document

Other files and links

Fingerprint

Cite this