sameAs
Cosmological parameters from SDSS and WMAPNeutrino physics from the cosmic microwave background and large scale structureDetection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPTBaryon-symmetric baryogenesisProbing Gravity at Cosmological Scales by Measurements which Test the Relationship between Gravitational Lensing and Matter OverdensitySterile neutrinos as dark matterIs Cosmology Compatible with Sterile Neutrinos?Primordial gravitational waves and cosmologySolving the coincidence problem: tracking oscillating energy.Size bias in galaxy surveys.Inference from the small scales of cosmic shear with current and future Dark Energy Survey dataCosmology from large-scale galaxy clustering and galaxy–galaxy lensing with Dark Energy Survey Science Verification dataJoint analysis of galaxy-galaxy lensing and galaxy clustering: Methodology and forecasts for Dark Energy SurveyCosmic shear measurements with Dark Energy Survey Science Verification dataCosmology from cosmic shear with Dark Energy Survey Science Verification dataNonlocal gravity and structure in the UniverseTHE REAL PROBLEM WITH MONDCan Cosmic Structure Form without Dark Matter?Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V ResultsCMB Polarization B-mode Delensing with SPTpol and HerschelSloan Digital Sky Survey: Early Data ReleaseCosmic Microwave Background Anisotropy Induced by Cosmic Strings on Angular Scales≳15′Reduced shear power spectrumGrowth of cosmic structure: Probing dark energy beyond expansionConstraining cosmological dark matter annihilation with gamma ray observationsExtracting the gamma ray signal from dark matter annihilation in the galactic center regionThe First Data Release of the Sloan Digital Sky SurveyOptimized clustering estimators for BAO measurements accounting for significant redshift uncertaintyCMB lensing tomography with the DES Science Verification galaxiesEight ultra-faint galaxy candidates discovered in year two of the dark energy surveyStellar kinematics and metallicities in the ultra-faint dwarf galaxy Reticulum IIGalaxy Clustering in Early Sloan Digital Sky Survey Redshift DataCosmological and astrophysical neutrino mass measurementsThe Sloan Digital Sky Survey coadd: 275 deg^2^ of deep Sloan Digital Sky Survey imaging on stripe 82Cross-correlation of gravitational lensing from DES Science Verification data with SPT andPlancklensingConstraints on the richness–mass relation and the optical-SZE positional offset distribution for SZE-selected clustersImprint of DES superstructures on the cosmic microwave backgroundJoint measurement of lensing–galaxy correlations using SPT and DES SV dataInflation physics from the cosmic microwave background and large scale structureAn integral field spectrograph for SNAP
P50
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P50
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Scott Dodelson
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Scott Dodelson
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P31
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