Showing 1–14 of 14 results
/ Date/ Name
Dec 20, 2012Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter ResultsDec 20, 2012Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and ResultsJan 26, 2010Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived ParametersNov 26, 2008Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization MapsMar 5, 2008Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window FunctionsApr 30, 2007Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground PolarizationMar 19, 2006Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for CosmologyFeb 11, 2003First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors LimitsFeb 11, 2003Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE PolarizationFeb 11, 2003First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window FunctionsFeb 11, 2003First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic ResultsJan 10, 2003The Microwave Anisotropy Probe (MAP) MissionMar 3, 1998The Spectrum of the Extragalactic Far Infrared Background from the COBE Firas ObservationsJul 10, 1996Gauge Couplings calculated from Multiple Point Criticality yield $α^{-1}=136._8\pm 9$: At Last the Elusive Case of $U(1)$