ACBAR measurements of CMB angular power spectrum

Kuo, C. L., Daub, M., Holzapfel, W., Newcomb, M., Goldstein, J., Ruhl, J., Torbet, E., Bock, J., Runyan, M., Peterson, J. and Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401 2002. ACBAR measurements of CMB angular power spectrum. Presented at: 200th Annual Meeting of the American Astronomical Society (AAS), Albuquerque, NM, USA, June 2002.

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Abstract

Arcminute Bolometer Array Receiver (ACBAR) is a 16-element bolometer array operating at 230mK. ACBAR was deployed at the South Pole in December 2000. Here we present the CMB angular power spectrum in the range 200<l<2200 measured by ACBAR during the austral winter of 2001.

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Completion
Status:	Unpublished
Schools:	Schools > Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Additional Information:	Abstract published in the Bulletin of the American Astronomical Society Vol 34 (No 2) 2002 Session 6. Cosmology, The Early Universe
Last Modified:	24 Oct 2022 10:06
URI:	https://orca.cardiff.ac.uk/id/eprint/43145

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