The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
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Cosmological parameters from SDSS and WMAPCosmological constraints from the SDSS luminous red galaxiesConfirmation of the Copernican Principle at Gpc Radial Scale and above from the Kinetic Sunyaev-Zel’dovich Effect Power SpectrumSearching for CPT violation with cosmic microwave background data from WMAP and BOOMERANGObservational constraints on dark energy and cosmic curvatureDark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?Indication for Primordial Anisotropies in the Neutrino Background from the Wilkinson Microwave Anisotropy Probe and the Sloan Digital Sky SurveyIs Cosmology Compatible with Sterile Neutrinos?The Hubble Constant.Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic ExtensionsMeasuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraintsConfirmation of the Copernican principle through the anisotropic kinetic Sunyaev Zel'dovich effect.Beyond two dark energy parameters.Neutrino masses and the dark energy equation of state: relaxing the cosmological neutrino mass bound.Initial conditions of the universe: how much isocurvature is allowed?Large Scale Structure in Bekenstein’s Theory of Relativistic Modified Newtonian DynamicsThe large-scale structure of the UniverseSimulating structure formation of the Local UniverseCan Cosmic Structure Form without Dark Matter?The effect of foreground subtraction on cosmological measurements from intensity mappingGalaxy halo masses and satellite fractions from galaxy-galaxy lensing in the Sloan Digital Sky Survey: stellar mass, luminosity, morphology and environment dependenciesProbing the nature of dark energy through galaxy redshift surveys with radio telescopesEvolution of the cosmic webDelayed recombination and standard rulersCosmological constraints in the presence of ionizing and resonance radiation at recombinationObservables sensitive to absolute neutrino masses: A reappraisal after WMAP 3-year and first MINOS resultsModel of inflationary cosmology without singularityThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functionsClustering of intermediate redshift quasars using the final SDSS III-BOSS sampleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samplesThe clustering of intermediate-redshift quasars as measured by the Baryon Oscillation Spectroscopic SurveyCosmological parameter forecasts for H i intensity mapping experiments using the angular power spectrumGOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxiesMultiple inflation and the WMAP “glitches”. II. Data analysis and cosmological parameter extractionThe 6dF Galaxy Survey: bulk flows on 50-70h-1Mpc scalesThe WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9Extracting the gamma ray signal from dark matter annihilation in the galactic center regionThe VIMOS Public Extragalactic Redshift Survey (VIPERS)The clustering of luminous red galaxies in the Sloan Digital Sky Survey imaging dataCosmological constraints on f(R) gravity theories within the Palatini approach
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The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Mai 2004 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
@nl
наукова стаття, опублікована в травні 2004
@uk
name
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@en
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@nl
type
label
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@en
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@nl
prefLabel
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@en
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@nl
P2093
P50
P356
P1476
The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey
@en
P2093
Adrian Pope
Albert Stebbins
Andreas Berlind
Andrew J. S. Hamilton
Bhuvnesh Jain
Brian C. Lee
Brian Yanny
Christopher Stoughton
Constance Rockosi
Daniel E. Vanden Berk
P304
P356
10.1086/382125
P407
P50
P577
2004-05-10T00:00:00Z
P818
astro-ph/0310725
P819
2004ApJ...606..702T