Published January 5, 2006
| Accepted Version
Book Section - Chapter
Open
Star Forming Galaxies in the 'Redshift Desert'
- Others:
- Renzini, Alvio
- Bender, Ralf
Chicago
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Abstract
We describe results of optical and near-IR observations of a large spectroscopic sample of star-forming galaxies photometrically-selected to lie in the redshift range 1.4≾z≾2.5, often called the "redshift desert" because of historical difficulty in obtaining spectroscopic redshifts in this range. We show that the former "redshift desert" is now very much open to observation.
Additional Information
© Springer-Verlag Berlin Heidelberg 2005. More quantitative results in the areas discussed above, and analyses of the clustering properties, luminosity functions, and the relationship to and interaction with the diffuse IGM are all in preparation. We would like to thank the David and Lucile Packard Foundation and the US National Science Foundation for support for this workAttached Files
Accepted Version - 0401061.pdf
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Additional details
- Eprint ID
- 98241
- DOI
- 10.1007/10995020_26
- Resolver ID
- CaltechAUTHORS:20190826-124740287
- David and Lucile Packard Foundation
- NSF
- Created
-
2019-08-26Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- ESO Astrophysics Symposia