The NAture of the Faint Far-Infrared Extragalactic Source Population: Optical/NIR and Radio Follow-Up Observationts of ISOPHOT Deep-Field Sources using the Keck, Subaru, and VLA Telescopes.

Authors

Y Kakazu
DB Sanders
RD Joseph
LL Cowie
T Murayama
Y Taniguchi
S Veilleux
Min Yun, University of Massachusetts - AmherstFollow
K Kawara
Y Sofue
Y Sato
H Okuda
K Wakamatsu
T Matsumoto
H Matsuhara

Publication Date

2002

Journal or Book Title

Astronomical Society of the Pacific Conference Series

Abstract

In order to search for obscured objects at high redshifts, we have made deep far-infrared (FIR) deep survey in the Lockman Hole using ISOPHOT onboard ISO (Kawara et al. 1998, A&A, 336, L9). In this survey several tens of FIR sources have been found at 95micron and 175micron. Here we present results of optical and NIR spectroscopic followup observations performed at the W. M.Keck Observatory.

Comments

This is the pre-published version harvested from ArXiv. The published version is located at http://www.aspbooks.org/a/volumes/article_details/?paper_id=26011

DOI

https://doi.org/10.1017/S0252921100030700

Pages

213

Volume

284

Issue

AGN Surveys, IAU Colloquium 184

Recommended Citation

Kakazu, Y; Sanders, DB; Joseph, RD; Cowie, LL; Murayama, T; Taniguchi, Y; Veilleux, S; Yun, Min; Kawara, K; Sofue, Y; Sato, Y; Okuda, H; Wakamatsu, K; Matsumoto, T; and Matsuhara, H, "The NAture of the Faint Far-Infrared Extragalactic Source Population: Optical/NIR and Radio Follow-Up Observationts of ISOPHOT Deep-Field Sources using the Keck, Subaru, and VLA Telescopes." (2002). Astronomical Society of the Pacific Conference Series. 1116.
https://doi.org/10.1017/S0252921100030700