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Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common

Hayward, Christopher C. and Chapman, Scott C. and Steidel, Charles C. and Golob, Anneya and Casey, Caitlin M. and Smith, Daniel J. B. and Zitrin, Adi and Blain, Andrew W. and Bremer, Malcolm N. and Chen, Chian-Chou and Coppin, Kristen E. K. and Farrah, Duncan and Ibar, Eduardo and Michałowski, Michał J. and Sawicki, Marcin and Scott, Douglas and van der Werf, Paul and Fazio, Giovanni G. and Geach, James E. and Gurwell, Mark and Petitpas, Glen and Wilner, David J. (2018) Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common. Monthly Notices of the Royal Astronomical Society, 476 (2). pp. 2278-2287. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20180509-152638878

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Abstract

Interferometric observations have demonstrated that a significant fraction of single-dish submillimetre (submm) sources are blends of multiple submm galaxies (SMGs), but the nature of this multiplicity, i.e. whether the galaxies are physically associated or chance projections, has not been determined. We performed spectroscopy of 11 SMGs in six multicomponent submm sources, obtaining spectroscopic redshifts for nine of them. For an additional two component SMGs, we detected continuum emission but no obvious features. We supplement our observed sources with four single-dish submm sources from the literature. This sample allows us to statistically constrain the physical nature of single-dish submm source multiplicity for the first time. In three (3/7, or 43^(+39__(−33) per cent at 95 percent confidence) of the single-dish sources for which the nature of the blending is unambiguous, the components for which spectroscopic redshifts are available are physically associated, whereas 4/7 (57^(+33)_(−39) per cent) have at least one unassociated component. When components whose spectra exhibit continuum but no features and for which the photometric redshift is significantly different from the spectroscopic redshift of the other component are also considered, 6/9 (67^(+26)_(−37) per cent) of the single-dish sources are comprised of at least one unassociated component SMG. The nature of the multiplicity of one single-dish source is ambiguous. We conclude that physically associated systems and chance projections both contribute to the multicomponent single-dish submm source population. This result contradicts the conventional wisdom that bright submm sources are solely a result of merger-induced starbursts, as blending of unassociated galaxies is also important.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/sty304DOIArticle
https://arxiv.org/abs/1802.00452arXivDiscussion Paper
ORCID:
AuthorORCID
Hayward, Christopher C.0000-0003-4073-3236
Steidel, Charles C.0000-0002-4834-7260
Casey, Caitlin M.0000-0002-0930-6466
Zitrin, Adi0000-0002-0350-4488
Blain, Andrew W.0000-0001-7489-5167
Chen, Chian-Chou0000-0002-3805-0789
Farrah, Duncan0000-0003-1748-2010
Michałowski, Michał J.0000-0001-9033-4140
Sawicki, Marcin0000-0002-7712-7857
Scott, Douglas0000-0002-6878-9840
van der Werf, Paul0000-0001-5434-5942
Fazio, Giovanni G.0000-0002-0670-0708
Geach, James E.0000-0003-4964-4635
Gurwell, Mark0000-0003-0685-3621
Wilner, David J.0000-0003-1526-7587
Additional Information:© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2018 February 1. Received 2018 January 29; in original form 2017 August 25. Published: 09 February 2018. CCH thanks Nick Scoville for encouragement to try his hand at observing, Ian Smail for inspiration via his Fifth Rule of Observational Cosmology (If you see an observational paper with a theorist as lead author be very afraid), and Allison Strom for advice when planning the observations. We also thank James Simpson and Ian Smail for comments on an earlier version of the manuscript, Mark Swinbank for useful discussion, and the anonymous referee for useful comments that led us to improve the manuscript. The Flatiron Institute is supported by the Simons Foundation. Some of this work was supported by a National Aeronautics and Space Administration (NASA) Keck PI Data Award, administered by the NASA Exoplanet Science Institute. EI acknowledges partial support from Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT) through grant no.  1171710. MJM acknowledges the support of the National Science Centre, Poland through POLONEZ grant 2015/19/P/ST9/04010. This project has received funding from the European Union's Horizon 2020 research and innovation programme under Marie Skłodowska-Curie grant agreement no.  665778. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and NASA. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Partially based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation (NSF) on behalf of the Gemini partnership: the NSF (United States), the National Research Council (Canada), Comisión Nacional de Investigación Científica y Tecnológica (CONICYT) (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil). This research has made use of the NASA/Infrared Processing and Analysis Center (IPAC) Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, the VizieR data base of astronomical catalogues (Ochsenbein, Bauer & Marcout 2000), NASA’s Astrophysics Data System Bibliographic Services, the arXiv.org preprint server, and ASTROPY, a community-developed core PYTHON package for astronomy (Astropy Collaboration 2013).
Funders:
Funding AgencyGrant Number
Simons FoundationUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)1171710
National Science Centre (Poland)2015/19/P/ST9/04010
Marie Curie Fellowship665778
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:galaxies: high-redshift – galaxies: starburst – infrared: galaxies – submillimetre: galaxies
Issue or Number:2
Record Number:CaltechAUTHORS:20180509-152638878
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180509-152638878
Official Citation:Christopher C Hayward, Scott C Chapman, Charles C Steidel, Anneya Golob, Caitlin M Casey, Daniel J B Smith, Adi Zitrin, Andrew W Blain, Malcolm N Bremer, Chian-Chou Chen, Kristen E K Coppin, Duncan Farrah, Eduardo Ibar, Michał J Michałowski, Marcin Sawicki, Douglas Scott, Paul van der Werf, Giovanni G Fazio, James E Geach, Mark Gurwell, Glen Petitpas, David J Wilner; Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common, Monthly Notices of the Royal Astronomical Society, Volume 476, Issue 2, 11 May 2018, Pages 2278–2287, https://doi.org/10.1093/mnras/sty304
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:86323
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 May 2018 17:11
Last Modified:01 Nov 2019 20:39

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