T.M. Hughes
VALES: III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies
Hughes, T.M.; Ibar, E.; Villaneuva, 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.; van Kampen, E.; Lara-Lopez, M.A.; Maddox, S.; Micha?owski, M.J.; Oteo, I.; Smith, D.; Smith, M.W.L.; Valiante, E.; van der Werf, Paul; Viaene, S.; Xue, Y.Q.
Authors
E. Ibar
V. Villaneuva
M. Aravena
M. Baes
N. Bourne
A. Cooray
L.J.M. Davies
S. Driver
L. Dunne
SIMON DYE Simon.Dye@nottingham.ac.uk
Professor of Astrophysics
S. Eales
C. Furlanetto
R. Herrera-Camus
R.J. Ivison
E. van Kampen
M.A. Lara-Lopez
S. Maddox
M.J. Micha?owski
I. Oteo
D. Smith
M.W.L. Smith
E. Valiante
Paul van der Werf
S. Viaene
Y.Q. Xue
Abstract
We present the calibration between the dust continuum luminosity and interstellar gas content obtained from the Valparaiso 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−1Θ, in excellent agreement with literature values. We obtain a linear fit of log10 (MH2/MΘ) = (0.92 ± 0.02) log10(Lν850 /erg s−1 Hz−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.
Citation
Hughes, T., Ibar, E., Villaneuva, V., Aravena, M., Baes, M., Bourne, N., …Xue, Y. (2017). VALES: III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 468(1), L103-L107. https://doi.org/10.1093/mnrasl/slx033
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 23, 2017 |
Publication Date | Feb 27, 2017 |
Deposit Date | May 2, 2017 |
Publicly Available Date | May 2, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 468 |
Issue | 1 |
Article Number | L103-L107 |
Pages | L103-L107 |
DOI | https://doi.org/10.1093/mnrasl/slx033 |
Keywords | ISM: lines and bands – galaxies: ISM – submillimetre: galaxies |
Public URL | https://nottingham-repository.worktribe.com/output/844121 |
Publisher URL | https://academic.oup.com/mnrasl/article/3055704/VALES: |
Additional Information | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Contract Date | May 2, 2017 |
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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
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