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The clustering of submillimeter galaxies detected with ALMA

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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The clustering of submillimeter galaxies detected with ALMA. / Garcia-Vergara, Cristina; Hodge, Jacqueline; Hennawi, Joseph F. et al.
In: The Astrophysical Journal, Vol. 904, No. 1, 2, 17.11.2020.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Garcia-Vergara, C, Hodge, J, Hennawi, JF, Weiss, A, Wardlow, J, Myers, AD & Hickox, R 2020, 'The clustering of submillimeter galaxies detected with ALMA', The Astrophysical Journal, vol. 904, no. 1, 2. https://doi.org/10.3847/1538-4357/abbdfe

APA

Garcia-Vergara, C., Hodge, J., Hennawi, J. F., Weiss, A., Wardlow, J., Myers, A. D., & Hickox, R. (2020). The clustering of submillimeter galaxies detected with ALMA. The Astrophysical Journal, 904(1), Article 2. https://doi.org/10.3847/1538-4357/abbdfe

Vancouver

Garcia-Vergara C, Hodge J, Hennawi JF, Weiss A, Wardlow J, Myers AD et al. The clustering of submillimeter galaxies detected with ALMA. The Astrophysical Journal. 2020 Nov 17;904(1):2. doi: 10.3847/1538-4357/abbdfe

Author

Garcia-Vergara, Cristina ; Hodge, Jacqueline ; Hennawi, Joseph F. et al. / The clustering of submillimeter galaxies detected with ALMA. In: The Astrophysical Journal. 2020 ; Vol. 904, No. 1.

Bibtex

@article{a6014276765f4a3cab872477770f9f50,
title = "The clustering of submillimeter galaxies detected with ALMA",
abstract = "Previous studies measuring the clustering of submillimeter galaxies (SMGs) have based their measurements on single-dish detected sources, finding evidence for strong clustering. However, ALMA has revealed that, due to the coarse angular resolution of these instruments, single-dish sources can be comprised of multiple sources. This implies that the clustering inferred from single-dish surveys may be overestimated. Here, we measure the clustering of SMGs based on the ALESS survey, an ALMA follow-up of sources previously identified in the LABOCA ECDFS Submillimeter Survey (LESS). We present a method to measure the clustering of ALMA sources that have been previously identified using single-dish telescopes, based on forward modeling both the single-dish and the ALMA observations. We constrain upper limits for the median mass of halos hosting SMGs at $1",
keywords = "Astrophysics - Astrophysics of Galaxies",
author = "Cristina Garcia-Vergara and Jacqueline Hodge and Hennawi, {Joseph F.} and Axel Weiss and Julie Wardlow and Myers, {Adam D.} and Ryan Hickox",
note = "This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/abbdfe",
year = "2020",
month = nov,
day = "17",
doi = "10.3847/1538-4357/abbdfe",
language = "English",
volume = "904",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - The clustering of submillimeter galaxies detected with ALMA

AU - Garcia-Vergara, Cristina

AU - Hodge, Jacqueline

AU - Hennawi, Joseph F.

AU - Weiss, Axel

AU - Wardlow, Julie

AU - Myers, Adam D.

AU - Hickox, Ryan

N1 - This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/abbdfe

PY - 2020/11/17

Y1 - 2020/11/17

N2 - Previous studies measuring the clustering of submillimeter galaxies (SMGs) have based their measurements on single-dish detected sources, finding evidence for strong clustering. However, ALMA has revealed that, due to the coarse angular resolution of these instruments, single-dish sources can be comprised of multiple sources. This implies that the clustering inferred from single-dish surveys may be overestimated. Here, we measure the clustering of SMGs based on the ALESS survey, an ALMA follow-up of sources previously identified in the LABOCA ECDFS Submillimeter Survey (LESS). We present a method to measure the clustering of ALMA sources that have been previously identified using single-dish telescopes, based on forward modeling both the single-dish and the ALMA observations. We constrain upper limits for the median mass of halos hosting SMGs at $1

AB - Previous studies measuring the clustering of submillimeter galaxies (SMGs) have based their measurements on single-dish detected sources, finding evidence for strong clustering. However, ALMA has revealed that, due to the coarse angular resolution of these instruments, single-dish sources can be comprised of multiple sources. This implies that the clustering inferred from single-dish surveys may be overestimated. Here, we measure the clustering of SMGs based on the ALESS survey, an ALMA follow-up of sources previously identified in the LABOCA ECDFS Submillimeter Survey (LESS). We present a method to measure the clustering of ALMA sources that have been previously identified using single-dish telescopes, based on forward modeling both the single-dish and the ALMA observations. We constrain upper limits for the median mass of halos hosting SMGs at $1

KW - Astrophysics - Astrophysics of Galaxies

U2 - 10.3847/1538-4357/abbdfe

DO - 10.3847/1538-4357/abbdfe

M3 - Journal article

VL - 904

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 2

ER -