An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 sub-millimetre galaxies

dc.contributor.authorAn, Fang Xia
dc.contributor.authorSmail, Ian
dc.contributor.authorSwinbank, A. M.
dc.date.accessioned2021-02-08T12:59:33Z
dc.date.available2021-02-08T12:59:33Z
dc.date.issued2020
dc.description.abstractWe analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ∼1 deg2 field, including ∼17 per cent, which are undetected at K ≳ 25.7 mag. We interpret their ultraviolet-to-radio data using MAGPHYS and determine a median redshift of z = 2.61 ± 0.08 (1σ range of z = 1.8–3.4) with just ∼6 per cent at z > 4. Our survey provides a sample of massive dusty galaxies at z ≳ 1, with median dust and stellar masses of Md = (6.8 ± 0.3) × 108 M⊙ (thus, gas masses of ∼1011 M⊙) and M* = (1.26 ± 0.05) × 1011 M⊙.en_US
dc.identifier.citationAn, F. X. et al. (2020). An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 sub-millimetre galaxies. Monthly Notices of the Royal Astronomical Society, 494(3), 3828–3860en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/staa769
dc.identifier.urihttp://hdl.handle.net/10566/5867
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxies: high-redshiften_US
dc.subjectGalaxies: starbursten_US
dc.subjectSubmillimetre: galaxiesen_US
dc.subjectALMA surveyen_US
dc.subjectSCUBA-2en_US
dc.titleAn ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 sub-millimetre galaxiesen_US
dc.typeArticleen_US

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