Authors
Peter AR Ade, Z Ahmed, RW Aikin, KD Alexander, D Barkats, SJ Benton, Colin A Bischoff, JJ Bock, Rachel Bowens-Rubin, JA Brevik, I Buder, E Bullock, Victor Buza, J Connors, BP Crill, L Duband, Cora Dvorkin, JP Filippini, S Fliescher, J Grayson, M Halpern, Sarah Harrison, GC Hilton, H Hui, KD Irwin, Kirit Sukrit Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, John M Kovac, CL Kuo, EM Leitch, M Lueker, KG Megerian, CB Netterfield, HT Nguyen, R O’Brient, RW Ogburn IV, A Orlando, C Pryke, S Richter, R Schwarz, CD Sheehy, ZK Staniszewski, B Steinbach, RV Sudiwala, GP Teply, KL Thompson, JE Tolan, C Tucker, AD Turner, AG Vieregg, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, KW Yoon, (Keck Array and BICEP2 Collaborations)
Publication date
2016/1/22
Journal
Physical Review Letters
Volume
116
Issue
3
Pages
031302
Publisher
American Physical Society
Description
We present results from an analysis of all data taken by the BICEP2 and Keck Array cosmic microwave background (CMB) polarization experiments up to and including the 2014 observing season. This includes the first Keck Array observations at 95 GHz. The maps reach a depth of 50 nK deg in Stokes and in the 150 GHz band and 127 nK deg in the 95 GHz band. We take auto- and cross-spectra between these maps and publicly available maps from WMAP and Planck at frequencies from 23 to 353 GHz. An excess over lensed is detected at modest significance in the spectrum, and is consistent with the dust contribution expected from our previous work. No significant evidence for synchrotron emission is found in spectra such as , or for correlation between the dust and synchrotron sky patterns in spectra such as . We take the likelihood of all the spectra for a multicomponent model including lensed …
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