Radio Properties of EROs in the Phoenix Deep Survey
Astrophysics
2007-05-23 v1
Abstract
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 a sample of star-forming extremely red objects (EROs). Stacking of the radio images of the radio-undetected star-forming EROs revealed a significant radio detection. Using the expected median redshift, we estimate an average star-formation rate of 61 M_sun/yr for these galaxies.
Keywords
Cite
@article{arxiv.astro-ph/0312117,
title = {Radio Properties of EROs in the Phoenix Deep Survey},
author = {J. Afonso and A. M. Hopkins and M. Sullivan and B. Mobasher and A. Georgakakis and L. E. Cram},
journal= {arXiv preprint arXiv:astro-ph/0312117},
year = {2007}
}
Comments
2 pages, 2 figures, To be published in Proceedings of the ESO/USM/MPE Workshop on "Multiwavelength Mapping of Galaxy Formation and Evolution"