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A machine-learning method for identifying multiwavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS

An, Fang Xia; Stach, S.M.; Smail, Ian; Swinbank, A.M.; Almaini, O.; Simpson, C.; Hartley, W.; Maltby, D.T.; Ivison, R.J.; Arumugam, V.; Wardlow, J.L.; Cooke, E.A.; Gullberg, B.; Thomson, A.P.; Chen, Chian-Chou; Simpson, J.M.; Geach, J.E.; Scott, D.; Dunlop, J.S.; Farrah, D.; Werf, P. van der; Blain, A.W.; Conselice, C.; Michałowski, M.; Chapman, S.C.; Coppin, K.E.K.

A machine-learning method for identifying multiwavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS Thumbnail


Authors

Fang Xia An

S.M. Stach

Ian Smail

A.M. Swinbank

OMAR ALMAINI omar.almaini@nottingham.ac.uk
Professor of Astrophysics

C. Simpson

W. Hartley

R.J. Ivison

V. Arumugam

J.L. Wardlow

E.A. Cooke

B. Gullberg

A.P. Thomson

Chian-Chou Chen

J.M. Simpson

J.E. Geach

D. Scott

J.S. Dunlop

D. Farrah

P. van der Werf

A.W. Blain

C. Conselice

M. Michałowski

S.C. Chapman

K.E.K. Coppin



Abstract

We describe the application of supervised machine-learning algorithms to identify the likely multiwavelength counterparts to submillimeter sources detected in panoramic, single-dish submillimeter surveys. As a training set, we employ a sample of 695 (S870μm more than or approximate1 mJy) submillimeter galaxies(SMGs)with precise identifications from the ALMA follow-up of the SCUBA-2 Cosmology Legacy Survey’s UKIDSS-UDS field(AS2UDS). We show that radio emission, near-/mid-infrared colors, photometric redshift, and absolute H-band magnitude are effective predictors that can distinguish SMGs from submillimeter-faint field galaxies. Our combined radio + machine-learning method is able to successfully recover ∼85% of ALMA-identified SMGs that are detected in at least three bands from the ultraviolet to radio. We confirm the robustness of our method by dividing our training set into independent subsets and using these for training and testing, respectively, as well as applying our method to an independent sample of ∼100 ALMA-identified SMGs from the ALMA/LABOCA ECDF-South Survey(ALESS). To further test our methodology, we stack the 870 μm ALMA maps at the positions of those K-band galaxies that are classified as SMG counterparts by the machine learning but do not have a more than 4.3 σ ALMA detection. The median peak flux density of these galaxies is S870μm =(0.61 ± 0.03)mJy, demonstrating that our method can recover faint and/or diffuse SMGs even when they are below the detection threshold of our ALMA observations. In future, we will apply this method to samples drawn from panoramic single-dish submillimeter surveys that currently lack interferometric follow-up observations to address science questions that can only be tackled with large statistical samples of SMGs.

Citation

An, F. X., Stach, S., Smail, I., Swinbank, A., Almaini, O., Simpson, C., …Coppin, K. (2018). A machine-learning method for identifying multiwavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS. Astrophysical Journal, 862(2), Article 101. https://doi.org/10.3847/1538-4357/aacdaa

Journal Article Type Article
Acceptance Date Jun 17, 2018
Online Publication Date Jul 27, 2018
Publication Date Aug 1, 2018
Deposit Date Sep 7, 2018
Publicly Available Date Mar 28, 2024
Journal The Astrophysical Journal
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 862
Issue 2
Article Number 101
DOI https://doi.org/10.3847/1538-4357/aacdaa
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://nottingham-repository.worktribe.com/output/1065355
Publisher URL http://iopscience.iop.org/article/10.3847/1538-4357/aacdaa

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