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PublicaciónPlanck 2018 results. VI. Cosmological parameters (Corrigendum)
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PublicaciónPlanck 2018 results. VIII. Gravitational lensing
We present measurements of the cosmic microwave background (CMB) lensing potential using the final Planck 2018 temperature and polarization data. Using...
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PublicaciónPlanck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
The six parameters of the standard ΛCDM model have best-fit values derived from the Planck temperature power spectrum that are shifted somewhat from the best...
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PublicaciónPlanck intermediate results. LVII. Joint Planck LFI and HFI data processing
We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency...
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PublicaciónPlanck intermediate results. XLIX. Parity-violation constraints from polarization data
Parity-violating extensions of the standard electromagnetic theory cause in vacuo rotation of the plane of polarization of propagating photons. This effect...
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PublicaciónPlanck intermediate results. XVI. Profile likelihoods for cosmological parameters
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit). This allows a refinement of the ΛCDM best-fit...
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PublicaciónPlanck intermediate results. XXIV. Constraints on variations in fundamental constants
Any variation in the fundamental physical constants, more particularly in the fine structure constant, α, or in the mass of the electron, me, affects the...
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PublicaciónProbing gravity with the DES-CMASS sample and BOSS spectroscopy
The DES-CMASS sample (DMASS) is designed to optimally combine the weak lensing measurements from the Dark Energy Survey (DES) and redshift-space distortions...
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PublicaciónRedshift-distance relations from type Ia supernova observations. New constraints on grey dust models
Extinction due to intergalactic grey dust has been proposed as an alternative to accelerated expansion to account for the dimming of SnIa fluxes beyond z ≃ 0.5...