Clustering in the Caltech Faint Galaxy Redshift Survey

Cohen, Judith (2000) Clustering in the Caltech Faint Galaxy Redshift Survey. In: Clustering at High Redshift. Astronomical Society of the Pacific Conference Series. No.200. Astronomical Society of the Pacific , San Francisco, CA, pp. 314-318. ISBN 9781583810279. https://resolver.caltech.edu/CaltechAUTHORS:20190524-104736397

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Abstract

The Caltech Faint Galaxy Redshift Survey has collected ∼2000 spectra taken with multi-slit masks using the Low Resolution Imaging Spectrograph at the Keck Observatory (Oke et al 1995) in two widely separated fields on the sky, each ∼1 x 1 deg^2. Most of these objects are faint field galaxies; about 10% are Galactic stars and about 1% are broad-lined AGNs. I summarize the small scale clustering of this sample as well as the evidence in support of large scale structure.

Item Type:

Book Section

Related URLs:

URL	URL Type	Description
http://www.aspbooks.org/a/volumes/article_details/?paper_id=19244	Publisher	Article
http://adsabs.harvard.edu/abs/2000ASPC..200..314C	ADS	Article
https://arxiv.org/abs/astro-ph/9910242	arXiv	Discussion Paper

ORCID:

Author	ORCID
Cohen, Judith	0000-0002-8039-4673

Additional Information:

© 2000 Astronomical Society of the Pacific. Provided by the NASA Astrophysics Data System. I thank my collaborators Roger Blandford of Caltech and David Hogg of the Institute for Advanced Study, with whom most of this work was done. I am grateful for partial support from STScI/NASA grant AR-06337.12-94A.

Funders:

Funding Agency	Grant Number
NASA	AR-06337.12-94A

Series Name:

Astronomical Society of the Pacific Conference Series

Issue or Number:

200

Record Number:

CaltechAUTHORS:20190524-104736397

Persistent URL:

https://resolver.caltech.edu/CaltechAUTHORS:20190524-104736397

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No commercial reproduction, distribution, display or performance rights in this work are provided.

ID Code:

95785

Collection:

CaltechAUTHORS

Deposited By:

Tony Diaz

Deposited On:

24 May 2019 18:02

Last Modified:

03 Oct 2019 21:16

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