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A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B

Chapman, S. C. and Blain, A. and Ivison, R. and Smail, I. (1997) A Spectroscopic Survey of the Submillimeter Galaxy Population: 85 Redshifts Using Keck/LRIS-B. In: The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics. No.91. Springer , Berlin, pp. 15-21. ISBN 978-3-642-62348-6. https://resolver.caltech.edu/CaltechAUTHORS:20200325-142553056

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Abstract

We present spectroscopic identifications for a sample of 85 millimeter and submillimeter galaxies detected with the SCUBA/JCMT and MAMBO/IRAM-30m facilities, all identified with deep 1.4GHz VLA radio observations. The galaxies lie at redshifts z = 0.5 to 3.5, we describe their properties, especially the presence of active galactic nuclei (AGN) in the sample, and discuss the connection of the mm/submm galaxies and the formation of spheroidal components of galaxies, which requires knowledge of the timescales of their very luminous activity. For a subset of the galaxies, we show their disturbed and diverse Hubble Space Telescope (HST) optical morphologies.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-3-642-18902-9_3DOIArticle
https://rdcu.be/b3exAPublisherFree ReadCube access
ORCID:
AuthorORCID
Blain, A.0000-0001-7489-5167
Ivison, R.0000-0001-5118-1313
Smail, I.0000-0003-3037-257X
Additional Information:© 1997 Springer-Verlag Berlin Heidelberg.
Subject Keywords:Star Formation; Active Galactic Nucleus; Hubble Space Telescope; Radio Observation; Redshift Distribution
Series Name:Springer Proceedings in Physics
Issue or Number:91
DOI:10.1007/978-3-642-18902-9_3
Record Number:CaltechAUTHORS:20200325-142553056
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200325-142553056
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:102109
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Mar 2020 22:15
Last Modified:16 Nov 2021 18:08

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