Observing the CMB at High-l using the VSA and AMI

Details Observing the CMB at High-l using the VSA and AMI Observing the CMB at High-l using the VSA and AMI

2003-05-26

arxiv.org/abs/astro-ph/0305485v1

Astronomy and Astrophysics

Astrophysics

8 pages, 13 figures. To be published in the proceedings of "The Cosmic Microwave Background and its Polarization", New Astrono

Scientific paper

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-Zel'dovich effect. The combined l-range of these two instruments is between l = 150 and ~10000.

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