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dc.contributor.authorHughes, T. M.
dc.contributor.authorIbar, E.
dc.contributor.authorVillanueva, V.
dc.contributor.authorAravena, M.
dc.contributor.authorBaes, M.
dc.contributor.authorBourne, N.
dc.contributor.authorCooray, A.
dc.contributor.authorDavies, L. J. M.
dc.contributor.authorDriver, S.
dc.contributor.authorDunne, L.
dc.contributor.authorDye, S.
dc.contributor.authorEales, S.
dc.contributor.authorFurlanetto, C.
dc.contributor.authorHerrera-Camus, R.
dc.contributor.authorIvison, R. J.
dc.contributor.authorKampen, E. van
dc.contributor.authorLara-López, M. A.
dc.contributor.authorMaddox, S.
dc.contributor.authorMichałowski, M. J.
dc.contributor.authorOteo, I.
dc.contributor.authorSmith, D.
dc.contributor.authorSmith, M. W. L.
dc.contributor.authorValiante, E.
dc.contributor.authorWerf, P. van der
dc.contributor.authorViaene, S.
dc.contributor.authorXue, Y. Q.
dc.date.accessioned2018-01-19T12:30:13Z
dc.date.available2018-01-19T12:30:13Z
dc.date.issued2017-06
dc.identifier252097448
dc.identifier35d25902-cb3b-4135-b1ec-4649e84f3170
dc.identifier85030477474
dc.identifier000410066800022
dc.identifier.citationHughes , T M , Ibar , E , Villanueva , V , Aravena , M , Baes , M , Bourne , N , Cooray , A , Davies , L J M , Driver , S , Dunne , L , Dye , S , Eales , S , Furlanetto , C , Herrera-Camus , R , Ivison , R J , Kampen , E V , Lara-López , M A , Maddox , S , Michałowski , M J , Oteo , I , Smith , D , Smith , M W L , Valiante , E , Werf , P V D , Viaene , S & Xue , Y Q 2017 , ' VALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 468 , no. 1 , pp. L103-L107 . https://doi.org/10.1093/mnrasl/slx033en
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/1702.07350v1
dc.identifier.urihttps://hdl.handle.net/10023/12524
dc.description.abstractWe present the calibration between the dust continuum luminosity and interstellar gas content obtained from the Valparaíso ALMA Line Emission Survey (VALES) sample of 67 main-sequence star-forming galaxies at 0.02 < z < 0.35. We use CO(1–0) observations from the Atacama Large Millimetre/submillimetre Array to trace the molecular gas mass, MH2, and estimate the rest-frame monochromatic luminosity at 850 μm, Lν850, by extrapolating the dust continuum from magphys modelling of the far-ultraviolet to submillimetre spectral energy distribution sampled by the Galaxy And Mass Assembly survey. Adopting αCO = 6.5 (K km s−1 pc2)−1, the average ratio of Lν850/MH2 = (6.4 ± 1.4)× 1019 erg s−1 Hz−1 M−1⊙, in excellent agreement with literature values. We obtain a linear fit of log10(MH2/M⊙)=(0.92±0.02)log10(Lν850/ergs−1Hz−1)−(17.31±0.59). We provide relations between Lν850, MH2 and MISM when combining the VALES and literature samples, and adopting a Galactic αCO value.
dc.format.extent381155
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectISM: lines and bandsen
dc.subjectGalaxies: ISMen
dc.subjectSubmillimetre: galaxiesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleVALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxiesen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/mnrasl/slx033
dc.description.statusPeer revieweden
dc.identifier.urlhttp://arxiv.org/abs/1702.07350v1en


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