Show simple item record

Files in this item

Thumbnail

Item metadata

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.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.otherPURE: 252097448
dc.identifier.otherPURE UUID: 35d25902-cb3b-4135-b1ec-4649e84f3170
dc.identifier.otherArXiv: http://arxiv.org/abs/1702.07350v1
dc.identifier.otherScopus: 85030477474
dc.identifier.otherWOS: 000410066800022
dc.identifier.urihttp://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.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2017, the Author(s). This work has been made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at https://doi.org/10.1093/mnrasl/slx033en
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.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnrasl/slx033
dc.description.statusPeer revieweden
dc.identifier.urlhttp://arxiv.org/abs/1702.07350v1en


This item appears in the following Collection(s)

Show simple item record