## Abstract We describe the advantages of using Integral Field Spectroscopy to observe deep fields of galaxies. The VIMOS Integral Field Unit is particularly suitable for this kind of study thanks to its large fieldβofβview (βΌ1 arcmin^2^). After a short description of the VIMOSβIFU data reduction,
High redshift structures and the geometry of the universe
β Scribed by Steven Phillipps
- Publisher
- Springer Netherlands
- Year
- 1996
- Tongue
- English
- Weight
- 441 KB
- Volume
- 240
- Category
- Article
- ISSN
- 0004-640X
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