The Nature of the faint far-infrared extragalactic source population: Optical/NIR and radio follow-up observations of ISOPHOT deep-field sources using Keck, Subaru, and VLA telescopes

Simple item page
dc.creatorKakazu, Yuko
dc.creatorSanders, D. B.
dc.creatorJoseph, R. D.
dc.creatorCowie, L. L.
dc.creatorMurayama, T.
dc.creatorTaniguchi, Y.
dc.creatorVeilleux, S.
dc.creatorYun, M. S.
dc.creatorKawara, K.
dc.creatorSofue, Y.
dc.creatorSato, Y.
dc.creatorOkuda, H.
dc.creatorWakamatsu, K.
dc.creatorMatsumoto, T.
dc.date2002-01-21
dc.date.accessioned2026-07-07T02:02:18Z
dc.date.available2026-07-07T02:02:18Z
dc.descriptionWe report on optical and near-infrared (NIR) follow-up spectroscopy of faint far-infrared (FIR) sources found in our deep FIR survey by Kawara et al.
dc.description2 pages, 1 figure. To appear in the proceedings of "AGN Surveys" (IAU Colloquium 184)
dc.identifierhttps://arxiv.org/abs/astro-ph/0201326
dc.identifierhttp://arxiv.org/abs/astro-ph/0201326
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4036
dc.subjectAstrophysics
dc.titleThe Nature of the faint far-infrared extragalactic source population: Optical/NIR and radio follow-up observations of ISOPHOT deep-field sources using Keck, Subaru, and VLA telescopes
dc.typetext

Files

Collections

arXiv