Cosmological parameters from CMB and other data: A Monte Carlo approach
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Cosmological parameters from SDSS and WMAPExtending the generalized Chaplygin gas model by using geometrothermodynamicsPrecision cosmology defeats void models for accelerationConstraining fundamental physics with future CMB experimentsSignatures of relativistic neutrinos in CMB anisotropy and matter clusteringJoint analysis of BICEP2/keck array and Planck DataCosmological constraints from the SDSS luminous red galaxiesCosmological constraints on DGP braneworld gravity with brane tensionSuperimposed oscillations in the WMAP data?New constraints on variations of the fine structure constant from CMB anisotropiesSearching for CPT violation with cosmic microwave background data from WMAP and BOOMERANGObservational constraints on dark energy and cosmic curvatureCorrelation of CMB with large-scale structure. I. Integrated Sachs-Wolfe tomography and cosmological implicationsChallenges to the DGP model from horizon-scale growth and geometryFirst observational tests of eternal inflation: Analysis methods and WMAP 7-year resultsUpper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift SurveyNew Dark Energy Constraints from Supernovae, Microwave Background, and Galaxy ClusteringIndication for Primordial Anisotropies in the Neutrino Background from the Wilkinson Microwave Anisotropy Probe and the Sloan Digital Sky SurveyIs Cosmology Compatible with Sterile Neutrinos?Cosmology and Fundamental Physics with the Euclid Satellite.Forecast and analysis of the cosmological redshift drift.Quantifying the BICEP2-Planck tension over gravitational waves.Evidence for bouncing evolution before inflation after BICEP2.Joint cosmic microwave background and weak lensing analysis: constraints on cosmological parameters.Observing inflationary reheating.Cosmology based on f(R) gravity admits 1 eV sterile neutrinos.Examining the evidence for dynamical dark energy.Constraints on gravity on cosmic scales with upcoming large-scale structure surveys.Precise estimation of cosmological parameters using a more accurate likelihood function.Accelerating cosmologies from compactification.From Planck Data to Planck Era: Observational Tests of Holographic Cosmology.Cosmological constraints from type ia supernovae peculiar velocity measurements.Constraints from the Wilkinson microwave anisotropy probe on decaying cold dark matter.Cosmic voids and void lensing in the Dark Energy Survey Science Verification dataGalaxy–galaxy lensing in the Dark Energy Survey Science Verification dataCosmic shear measurements with Dark Energy Survey Science Verification dataH0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223:H0to 3.8 per cent precision from strong lensing in a flat ΛCDM modelTest of modified Newtonian dynamics with recent Boomerang dataTHE PHENOMENOLOGY OF RIGHT HANDED NEUTRINOSLow power on large scales in just-enough inflation models
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P2860
Cosmological parameters from CMB and other data: A Monte Carlo approach
description
2002 nî lūn-bûn
@nan
2002 թուականի Նոյեմբերին հրատարակուած գիտական յօդուած
@hyw
2002 թվականի նոյեմբերին հրատարակված գիտական հոդված
@hy
2002年の論文
@ja
2002年論文
@yue
2002年論文
@zh-hant
2002年論文
@zh-hk
2002年論文
@zh-mo
2002年論文
@zh-tw
2002年论文
@wuu
name
Cosmological parameters from CMB and other data: A Monte Carlo approach
@ast
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en-gb
type
label
Cosmological parameters from CMB and other data: A Monte Carlo approach
@ast
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en-gb
prefLabel
Cosmological parameters from CMB and other data: A Monte Carlo approach
@ast
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en-gb
P1433
P1476
Cosmological parameters from CMB and other data: A Monte Carlo approach
@en
P2093
Antony Lewis
P356
10.1103/PHYSREVD.66.103511
P407
P50
P577
2002-11-01T00:00:00Z
2002-11-25T00:00:00Z
P818
astro-ph/0205436