## 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 field‐of‐view (∼1 arcmin^2^). After a short description of the VIMOS‐IFU data reduction,
Observing the CMB at high-ℓ using the VSA and AMI
✍ Scribed by Angela C Taylor
- Book ID
- 103851555
- Publisher
- Elsevier Science
- Year
- 2003
- Tongue
- English
- Weight
- 370 KB
- Volume
- 47
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
✦ Synopsis
We discuss two experiments -the Very Small Array (VSA) and the Arcminute MicroKelvin Imager (AMI) -and their prospects for observing the CMB at high angular multipoles. Whilst the VSA is primarily designed to observe primary anisotropies in the CMB, AMI is designed to image secondary anisotropies via the Sunyaev-ZelÕdovich effect. The combined '-range of these two instruments is between ' ¼ 150 and $10,000.
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