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High-l CMB power spectrum from ACBAR: New results, observation status, and future prospects

Kuo, C. L., Ade, Peter A. R., Bock, J. J., Daub, M. D., Goldstein, J. H., Holzapfel, W. L., Lange, A. E., Lueker, M., Newcomb, M., Peterson, J. B., Reichardt, C., Ruhl, J., Runyan, M. C. and Staniszweski, Z. 2005. High-l CMB power spectrum from ACBAR: New results, observation status, and future prospects. Presented at: AAS 206th Meeting, Minneapolis, MN, 29 May - 2 June 2005.

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Abstract

We present new measurements of the temperature anisotropy in the cosmic microwave background using Arcminute Cosmology Bolometer Array Receiver (ACBAR). Significant improvements in sensitivity over previous data release were achieved by a combination of more efficient analysis techniques and the inclusion of more data. Together with the CBI measurements at lower photon frequencies, and the WMAP results on large angular scales, the joint ACBAR/CBI/WMAP power spectrum represents the current best knowledge of the temperature anisotropy between l=2 and 3000. Cosmological implications, current status of the instrument, and prospects for further improvements will be discussed.

Item Type: Conference or Workshop Item (Lecture)
Date Type: Completion
Status: Unpublished
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Additional Information: Session 21- Galaxies and Cosmology Abstract published in the Bulletin of the American Astronomical Society Vol 37 (2) in 2005
Last Modified: 04 Jun 2017 04:37
URI: http://orca.cf.ac.uk/id/eprint/41837

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