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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 the Keck, Subaru, and VLA Telescopes

Published online by Cambridge University Press:  12 April 2016

Yuko Kakazu
Affiliation:
Institute for Astronomy, University of Hawaii
D. B. Sanders
Affiliation:
Institute for Astronomy, University of Hawaii
R. D. Joseph
Affiliation:
Institute for Astronomy, University of Hawaii
L. L. Cowie
Affiliation:
Institute for Astronomy, University of Hawaii
T. Murayama
Affiliation:
Astronomical Institute, Tohoku Univesity
Y. Taniguchi
Affiliation:
Astronomical Institute, Tohoku Univesity
S. Veilleux
Affiliation:
Deptartment of Astronomy, University of Maryland
M. S. Yun
Affiliation:
FCRAO, University of Massachusetts
K. Kawara
Affiliation:
Institute of Astronomy, University of Tokyo
Y. Sofue
Affiliation:
Institute of Astronomy, University of Tokyo
Y. Sato
Affiliation:
Institute of Astronomy, University of Tokyo
H. Okuda
Affiliation:
Gumma Observatory
K. Wakamatsu
Affiliation:
Gifu University
T. Matsumoto
Affiliation:
ISAS.
H. Matsuhara
Affiliation:
ISAS.

Abstract

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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.

Type
Part 2. Infrared and Submillimeter Surveys for AGN
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Kawara, K., et al. 1998, A&A, 336, L9 Google Scholar
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Matsuhara, H., et al. 2000, A&A, 361, 407 Google Scholar
Murayama, T. & Taniguchi, Y. 1998, PASJ, 50, 241 Google Scholar
Yun, M.S., et al. 2002, in preparationGoogle Scholar