PPT-CMB large angular scale, full sky polarization anisotropy h

The value of reionization fraction derived from CMB polarization measurements has decreased steadily since WMAP2003 WMAP2005 WMAP2007 WMAP2011 and Planck 2015 The

planck cmb sky polarization cmb planck polarization sky foreground 100 large measured angular dust full spider emission noise bicep2

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