Dealing with beam structure in PIXIE
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Joseph M. Howard | Dale J. Fixsen | Lenward T. Seals | Alan J. Kogut | Peter C. Nagler | Robert S. Hill
[1] Kevin T. Crowley,et al. Multimode bolometer development for the PIXIE instrument , 2016, Astronomical Telescopes + Instrumentation.
[2] David N. Spergel,et al. The Primordial Inflation Explorer (PIXIE) , 2014, Astronomical Telescopes and Instrumentation.
[3] Nicolas Ponthieu,et al. CMB polarization systematics due to beam asymmetry: Impact on inflationary science , 2007, 0709.1513.
[4] Jacques Delabrouille,et al. Beam mismatch effects in Cosmic Microwave Background polarization measurements , 2004, astro-ph/0410544.
[5] D. J. Fixsen,et al. THE TEMPERATURE OF THE COSMIC MICROWAVE BACKGROUND , 2009, 0911.1955.
[6] M. Halpern,et al. Five-Year Wilkinson Microwave Anisotropy Probe (WMAP1) Observations: Galactic Foreground Emission , 2008 .
[7] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[8] M. Halpern,et al. The Primordial Inflation Explorer (PIXIE): a nulling polarimeter for cosmic microwave background observations , 2011, 1105.2044.
[9] C. A. Oxborrow,et al. Planck2015 results , 2015, Astronomy & Astrophysics.
[10] Giampaolo Pisano,et al. Removing beam asymmetry bias in precision CMB temperature and polarization experiments , 2014, 1401.2075.