Published September 26, 2003
| Version Submitted
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Deep Observations of Lyman Break Galaxies
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Abstract
We summarise the main results of recent work on the Lyman break galaxy population which takes advantage of newly commissioned instrumentation on the VLT and Keck telescopes to push the detection of these objects to new wavelengths and more sensitive limits.
Additional Information
© 2001 Springer-Verlag Berlin Heidelberg. First Online: 26 September 2003. Max Pettini would like to express his gratitude to the organisers of this enjoyable and timely meeting.Attached Files
Submitted - 0101254.pdf
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0101254.pdf
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Identifiers
- Eprint ID
- 103832
- DOI
- 10.1007/10854354_8
- Resolver ID
- CaltechAUTHORS:20200610-153115348
Related works
- Describes
- 10.1007/10854354_8 (DOI)
- https://arxiv.org/abs/astro-ph/0101254 (URL)
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- Created
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2020-06-10Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
Caltech Custom Metadata
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- ESO Astrophysics Symposia