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Planck 2013 results. I. Overview of products and scientific resultsThree‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for CosmologyNeutrino physics from the cosmic microwave background and large scale structurePlanck 2013 results. XVI. Cosmological parametersDetection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology TelescopeEvidence for Dark Energy from the Cosmic Microwave Background Alone Using the Atacama Cosmology Telescope Lensing MeasurementsEvidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel’dovich EffectFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP dataRecent discoveries from the cosmic microwave background: a review of recent progress.Evidence of lensing of the cosmic microwave background by dark matter halos.Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic resultsPlanck 2015 results. XIII. Cosmological parametersNine-year Wilkinson microwave anisotropy probe (WMAP) observations: final maps and resultsPlanck intermediate results XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudesFive-year Wilkinson Microwave Anisotropy Probe observations: cosmological interpretationSeven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: sky maps, systematic errors, and basic resultsThree‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Polarization AnalysisNine-year Wilkinson microwave anisotropy probe (WMAP) observations: cosmological parameter resultsThe Atacama Cosmology Telescope: CMB polarization at 200 < ℓ < 9000Probing Inflation with CMB PolarizationPlanck 2015 resultsSeven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: are there cosmic microwave background anomalies?Planck 2013 results. XXV. Searches for cosmic strings and other topological defectsModern methods for cosmological parameter estimation : beyond the adiabatic paradigmSeven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretationThe atacama cosmology telescope: a measurement of the 600 < {ell} < 8000 cosmic microwave background power spectrum at 148 GHzPlanck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dustPlanck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visiblePlanck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarizationPRISM (Polarized Radiation Imaging and Spectroscopy Mission): an extended white paperPlanck 2013 results. VI. High Frequency Instrument data processingPlanck 2013 results. VII. HFI time response and beamsPlanck 2013 results. XII. Diffuse component separationPlanck 2013 results. XV. CMB power spectra and likelihoodPlanck 2013 results. XVII. Gravitational lensing by large-scale structurePlanck 2013 results. XXII. Constraints on inflationPlanck 2013 results. XXIV. Constraints on primordial non-GaussianityPlanck early results. VI. The High Frequency Instrument data processingPlanck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parametersPlanck intermediate results XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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Jo Dunkley
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ஜோ தங்கிளே
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乔·邓克利
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