GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters

GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters

We compare common star formation rate (SFR) indicators in the local Universe in the Galaxy and Mass Assembly (GAMA) equatorial fields (∼160 deg2), using ultraviolet (UV) photometry from GALEX, far-infrared and sub-millimetre (sub-mm) photometry from Herschel Astrophysical Terahertz Large Area Survey...

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Bibliographic Details
Main Authors: Wang, L., Norberg, P., Gunawardhana, M.L.P., Heinis, S., Baldry, I.K., Bland-Hawthorn, J., Bourne, N., Brough, S., Brown, M.J.I., Cluver, M.E., Cooray, A., da Cunha, E., Driver, S.P., Dunne, L., Dye, S., Eales, S., Grootes, M.W., Holwerda, B.W., Hopkins, A.M., Ibar, E., Ivison, R., Lacey, C., Lara-Lopez, M.A., Loveday, J., Maddox, S.J., Michałowski, M.J., Oteo, I., Owers, M.S., Popescu, C.C., Smith, D.J.B., Taylor, E.N., Tuffs, R.J., van der Werf, P.
Format: Article
Published: Oxford University Press 2016
Subjects:
methods: statistical
galaxies: photometry
galaxies: statistics
infrared: galaxies
ultraviolet: galaxies
Online Access:https://eprints.nottingham.ac.uk/42348/

Internet

https://eprints.nottingham.ac.uk/42348/

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