Radio Properties of EROs in the Phoenix Deep Survey

(2) University of Pittsburgh; (3) University of Toronto; (4) STSCI; (5) National Athens Observatory; (6) Australian Research Council); A. Georgakakis (5); A. M. Hopkins (2); B. Mobasher (4); J. Afonso (1); L. E. Cram (6) ((1) CAAUL

arxiv: astro-ph/0312117 · v1 · submitted 2003-12-04 · 🌌 astro-ph

Radio Properties of EROs in the Phoenix Deep Survey

J. Afonso (1) , A. M. Hopkins (2) , M. Sullivan (3) , B. Mobasher (4) , A. Georgakakis (5) , L. E. Cram (6) ((1) CAAUL , Observatory of Lisbon , (2) University of Pittsburgh

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(3) University of Toronto (4) STSCI (5) National Athens Observatory (6) Australian Research Council)

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keywords radioerosstar-formingdeepdustgalaxiesphoenixsurvey

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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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Radio Properties of EROs in the Phoenix Deep Survey

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