Files in this item
VALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
Item metadata
dc.contributor.author | Hughes, T. M. | |
dc.contributor.author | Ibar, E. | |
dc.contributor.author | Villanueva, V. | |
dc.contributor.author | Aravena, M. | |
dc.contributor.author | Baes, M. | |
dc.contributor.author | Bourne, N. | |
dc.contributor.author | Cooray, A. | |
dc.contributor.author | Davies, L. J. M. | |
dc.contributor.author | Driver, S. | |
dc.contributor.author | Dunne, L. | |
dc.contributor.author | Dye, S. | |
dc.contributor.author | Eales, S. | |
dc.contributor.author | Furlanetto, C. | |
dc.contributor.author | Herrera-Camus, R. | |
dc.contributor.author | Ivison, R. J. | |
dc.contributor.author | Kampen, E. van | |
dc.contributor.author | Lara-López, M. A. | |
dc.contributor.author | Maddox, S. | |
dc.contributor.author | Michałowski, M. J. | |
dc.contributor.author | Oteo, I. | |
dc.contributor.author | Smith, D. | |
dc.contributor.author | Smith, M. W. L. | |
dc.contributor.author | Valiante, E. | |
dc.contributor.author | Werf, P. van der | |
dc.contributor.author | Viaene, S. | |
dc.contributor.author | Xue, Y. Q. | |
dc.date.accessioned | 2018-01-19T12:30:13Z | |
dc.date.available | 2018-01-19T12:30:13Z | |
dc.date.issued | 2017-06 | |
dc.identifier.citation | Hughes , 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/slx033 | en |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | PURE: 252097448 | |
dc.identifier.other | PURE UUID: 35d25902-cb3b-4135-b1ec-4649e84f3170 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1702.07350v1 | |
dc.identifier.other | Scopus: 85030477474 | |
dc.identifier.other | WOS: 000410066800022 | |
dc.identifier.uri | https://hdl.handle.net/10023/12524 | |
dc.description.abstract | We 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.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en |
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/slx033 | en |
dc.subject | ISM: lines and bands | en |
dc.subject | Galaxies: ISM | en |
dc.subject | Submillimetre: galaxies | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | 3rd-DAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | VALES - III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies | en |
dc.type | Journal article | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1093/mnrasl/slx033 | |
dc.description.status | Peer reviewed | en |
dc.identifier.url | http://arxiv.org/abs/1702.07350v1 | en |
This item appears in the following Collection(s)
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.