Radio Properties of EROs in the Phoenix Deep Survey

Details Radio Properties of EROs in the Phoenix Deep Survey Radio Properties of EROs in the Phoenix Deep Survey

2003-12-04

arxiv.org/abs/astro-ph/0312117v1

Astronomy and Astrophysics

Astrophysics

2 pages, 2 figures, To be published in Proceedings of the ESO/USM/MPE Workshop on "Multiwavelength Mapping of Galaxy Formation

Scientific paper

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.

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