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

D. B. Sanders; H. Okuda (Gumma Observatory); K. Kawara; K. Wakamatsu (Gifu Univ); L. L. Cowie (IfA; M. S. Yun (Univ of Massachusetts); R. D. Joseph; S. Veilleux (Univ of Maryland); T. Matsumoto (ISAS); T. Murayama

arxiv: astro-ph/0201326 · v1 · submitted 2002-01-21 · 🌌 astro-ph

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

Yuko Kakazu , D. B. Sanders , R. D. Joseph , L. L. Cowie (IfA , Univ of Hawaii) , T. Murayama , Y. Taniguchi (Tohoku Univ) , S. Veilleux (Univ of Maryland)

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M. S. Yun (Univ of Massachusetts) K. Kawara Y. Sofue Y. Sato (Univ of Tokyo) H. Okuda (Gumma Observatory) K. Wakamatsu (Gifu Univ) T. Matsumoto (ISAS)

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keywords faintfar-infraredfollow-upopticalsourcesdeepdeep-fieldextragalactic

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We 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.

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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

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