Galaxy And Mass Assembly: the 1.4 GHz SFR indicator, SFR-M* relation and predictions for ASKAP-GAMA
We present a robust calibration of the 1.4 GHz radio continuum star formation rate (SFR) using a combination of the Galaxy And Mass Assembly (GAMA) survey and the Faint Images of the Radio Sky at Twenty-cm (FIRST) survey. We identify individually detected 1.4 GHz GAMA–FIRST sources and use a late-ty...
| Main Authors: | Davies, L., Huynh, M., Hopkins, A., Seymour, Nick, Driver, S., Robotham, A., Baldry, I., Bland-Hawthorn, J., Bourne, N., Bremer, M., Brown, M., Brough, S., Cluver, M., Grootes, M., Jarvis, M., Loveday, J., Moffet, A., Owers, M., Phillipps, S., Sadler, E., Wang, L., Wilkins, S., Wright, A. |
|---|---|
| Format: | Journal Article |
| Published: |
Oxford University Press
2017
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| Online Access: | http://hdl.handle.net/20.500.11937/62913 |
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