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.
Cite
@article{arxiv.astro-ph/0107363,
title = {Observing the CMB with the AMiBA},
author = {Ravi Subrahmanyan},
journal= {arXiv preprint arXiv:astro-ph/0107363},
year = {2007}
}
Comments
6 pages, includes 2 figures, to appear in the ASP Conf Ser. proceedings of AMiBA 2001: High-z clusters, Missing baryons, and CMB polarization