Observing the CMB with the AMiBA
Abstract
I discuss the capabilities and limitations of the AMiBA for imaging CMB anisotropies. Michael Kesteven (ATNF-CSIRO) has proposed drift-scanning as an observing strategy for measuring and rejecting any instrumental response that the close-packed interferometers may have to the local environment. The advantages of mosaic imaging CMB anisotropies using a co-mounted interferometric array in a drift-scanning observing mode are discussed. A particular case of mosaic imaging a sky strip using a two-element AMiBA prototype interferometer is considered and the signal-to-noise ratio in the measurement of sky anisotropy using this observing strategy is analysed.
- Publication:
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AMiBA 2001: High-Z Clusters, Missing Baryons, and CMB Polarization
- Pub Date:
- 2002
- DOI:
- arXiv:
- arXiv:astro-ph/0107363
- Bibcode:
- 2002ASPC..257..309S
- Keywords:
-
- Astrophysics
- E-Print:
- 6 pages, includes 2 figures, to appear in the ASP Conf Ser. proceedings of AMiBA 2001: High-z clusters, Missing baryons, and CMB polarization