The Nature of the Faint Radio Population

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dc.creatorPrandoni, I.
dc.creatorGregorini, L.
dc.creatorParma, P.
dc.creatorde Ruiter, H. R.
dc.creatorVettolani, G.
dc.creatorWieringa, M.
dc.creatorEkers, R.
dc.date2001-09-10
dc.date.accessioned2026-07-07T01:59:54Z
dc.date.available2026-07-07T01:59:54Z
dc.descriptionWe present the results obtained so far from the optical follow-up of the ATESP sub-mJy radio survey. The ATESP results are then compared with the ones obtained from other deep radio samples and we show how the existing discrepancies about the nature of the faint radio population can be explained in terms of selection effects.
dc.description5 pages, 4 figures. To appear in Proc. of the Marseille 2001 Conference "Where's the Matter? Tracing dark and bright matter with the new generation of large scale surveys", 25-29 June 2001, Marseille (France)
dc.identifierhttps://arxiv.org/abs/astro-ph/0109143
dc.identifierhttp://arxiv.org/abs/astro-ph/0109143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3299
dc.subjectAstrophysics
dc.titleThe Nature of the Faint Radio Population
dc.typetext

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