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astro-ph2003
Radio Properties of EROs in the Phoenix Deep Survey
J. Afonso, A. M. Hopkins, M. Sullivan +3
Insensitive to dust obscuration, radio wavelengths are ideal to study star-forming galaxies free of dust induced biases. Using data from the Phoenix Deep Survey, we have identified…
astro-ph2003
The Phoenix Deep Survey: Evolution of Star Forming Galaxies
A. M. Hopkins, J. Afonso, A. Georgakakis +3
The Phoenix Deep Survey (PDS) is a multiwavelength survey based on deep 1.4 GHz radio observations used to identify a large sample of star forming galaxies to z=1. Photometric reds…
astro-ph2003
Two formation paths for cluster dwarf galaxies?
Bianca M. Poggianti, Nobunari Kashikawa, Terry Bridges +5
A surprising result of our recent spectroscopic survey of galaxies in the Coma cluster has been the discovery of a possible bimodal distribution in the metallicities of faint galax…