Authors
BS ea Mason, Timothy J Pearson, ACS Readhead, MC Shepherd, J Sievers, PS Udomprasert, JK Cartwright, AJ Farmer, S Padin, ST Myers, JR Bond, CR Contaldi, U Pen, S Prunet, D Pogosyan, JE Carlstrom, J Kovac, EM Leitch, C Pryke, NW Halverson, WL Holzapfel, P Altamirano, L Bronfman, S Casassus, J May, M Joy
Publication date
2003/7/10
Journal
The Astrophysical Journal
Volume
591
Issue
2
Pages
540
Publisher
IOP Publishing
Description
We report measurements of anisotropy in the cosmic microwave background radiation over the multipole range l∼ 200–3500 with the Cosmic Background Imager based on deep observations of three fields. These results confirm the drop in power with increasing l first reported in earlier measurements with this instrument and extend the observations of this decline in power out to l∼ 2000. The decline in power is consistent with the predicted damping of primary anisotropies. At larger multipoles, l= 2000–3500, the power is 3.1 σ greater than standard models for intrinsic microwave background anisotropy in this multipole range and 3.5 σ greater than zero. This excess power is not consistent with expected levels of residual radio source contamination but, for σ 8≳ 1, is consistent with predicted levels of a secondary Sunyaev-Zeldovich anisotropy. Further observations are necessary to confirm the level of this excess …
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Scholar articles
BS Mason, TJ Pearson, ACS Readhead, MC Shepherd… - The Astrophysical Journal, 2003