Revision history of "File:Results cosmo params vs uKarcmin FWHM.pdf"

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  • curprev 03:45, 19 May 2016Jerrard talk contribs 227 bytes +227 We look at the variation of cosmological constraints (neutrino mass, Neff, running and curvature) as a function of polarized sensitivity or resolution. We combine the one-channel CMB-S4 with Planck and/or DESI BAO measurements.