Radio Properties of EROs in the Phoenix Deep Survey

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dc.creatorAfonso, J.
dc.creatorHopkins, A. M.
dc.creatorSullivan, M.
dc.creatorMobasher, B.
dc.creatorGeorgakakis, A.
dc.creatorCram, L. E.
dc.date2003-12-04
dc.date.accessioned2026-07-07T02:11:26Z
dc.date.available2026-07-07T02:11:26Z
dc.descriptionInsensitive 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.
dc.description2 pages, 2 figures, To be published in Proceedings of the ESO/USM/MPE Workshop on "Multiwavelength Mapping of Galaxy Formation and Evolution"
dc.identifierhttps://arxiv.org/abs/astro-ph/0312117
dc.identifierhttp://arxiv.org/abs/astro-ph/0312117
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7082
dc.subjectAstrophysics
dc.titleRadio Properties of EROs in the Phoenix Deep Survey
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