Published 2000
| Published + Submitted
Book Section - Chapter
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Clustering in the Caltech Faint Galaxy Redshift Survey
- Creators
-
Cohen, Judith
- Others:
- Mazure, A.
- Le Fèvre, O.
- Le Brun, V.
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.
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.Attached Files
Published - 200-0314.pdf
Published - 2000ASPC__200__314C.pdf
Submitted - 9910242.pdf
Files
2000ASPC__200__314C.pdf
Additional details
- Eprint ID
- 95785
- Resolver ID
- CaltechAUTHORS:20190524-104736397
- AR-06337.12-94A
- NASA
- Created
-
2019-05-24Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific Conference Series
- Series Volume or Issue Number
- 200