The Phoenix deep survey: optical and near infrared imaging catalogs
The Phoenix Deep Survey is a multiwavelength galaxy survey based on deep 1.4 GHz radio imaging. The primary goal of this survey is to investigate the properties of star formation in galaxies and to trace the evolution in those properties to a redshift z = 1, covering a significant fraction of the age of the universe. By compiling a sample of star-forming galaxies based on selection at radio wavelengths we eliminate possible biases due to dust obscuration, a significant issue when selecting...[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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