VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35

VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35

We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterize galaxy populations up to z = 0.35: the Valpara´ıso ALMA Line Emission Survey (VALES). We use ALMA Band-3 CO(1–0) observations to study the molecular gas content in a sam...

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Bibliographic Details
Main Authors: Villanueva, V., Ibar, E., Hughes, T.M., Lara-Lopez, M.A., Dunne, L., Eales, S., Ivison, R.J., Aravena, M., Baes, M., Bourne, N., Cassata, P., Cooray, A., Dannerbauer, H., Davies, L.J.M., Driver, S.P., Dye, S., Furlanetto, C., Herrera-Camus, R., Maddox, S.J., Michałowski, M.J., Molina, J., Riechers, D., Sansom, A.E., Smith, M.W.L., Rodighiero, G., Valiante, E., van der Werf, P.
Format: Article
Language:English
Published: Oxford University Press 2017
Subjects:
ISM: lines and bands
galaxies: high-redshift
galaxies: ISM
infrared: galaxies
submillimetre: galaxies
Online Access:https://eprints.nottingham.ac.uk/45138/

Internet

https://eprints.nottingham.ac.uk/45138/

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