Consistently large cosmic flows on scales of100 h−1 Mpc: a challenge for the standard ΛCDM cosmology
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Peculiar motions, accelerated expansion, and the cosmological axisModified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic ExtensionsRe-examination of globally flat space-time.Cosmology and Fundamental Physics with the Euclid Satellite.Excess clustering on large scales in the MegaZ DR7 photometric redshift survey.Signature of local motion in the microwave sky.A structure in the early Universe at z ∼ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmologyDiscovery of a supercluster in the Zone of Avoidance in VelaPlanck intermediate results XIII. Constraints on peculiar velocitiesCosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density fieldCosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density fieldFirst measurement of the bulk flow of nearby galaxies using the cosmic microwave backgroundCosmic flows in the nearby universe from Type Ia supernovaeThe 2M++ galaxy redshift catalogueCosmic smoothnessHigh-redshift radio galaxies and divergence from the CMB dipoleProbing the anisotropic local Universe and beyond with SNe Ia dataThe 6dF Galaxy Survey: bulk flows on 50-70h-1Mpc scalesAre peculiar velocity surveys competitive as a cosmological probe?Cosmological constraints on dark energyDeriving accurate peculiar velocities (even at high redshift)The 6dF Galaxy Survey: cosmological constraints from the velocity power spectrumMeasuring cosmic bulk flows with Type Ia supernovae from the Nearby Supernova Factory2MTF – V. Cosmography, β, and the residual bulk flowInterpreting large-scale redshift-space distortion measurementsGalaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06The cosmic velocity fieldCosmic bulk flows on 50 h−1 Mpc scales: a Bayesian hyper-parameter method and multishell likelihood analysisA comparison of the galaxy peculiar velocity field with the PSCz gravity field - a Bayesian hyper-parameter methodTilted physics: A cosmologically dipole-modulated skyConstraining anisotropy of the universe from different groups of type-Ia supernovae
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Consistently large cosmic flows on scales of100 h−1 Mpc: a challenge for the standard ΛCDM cosmology
description
im Januar 2009 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в січні 2009
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name
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@en
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
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type
label
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@en
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@nl
prefLabel
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@en
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@nl
P1476
Consistently large cosmic flow ...... or the standard ΛCDM cosmology
@en
P2093
Hume A. Feldman
Richard Watkins
P304
P356
10.1111/J.1365-2966.2008.14089.X
P407
P577
2009-01-11T00:00:00Z
P818
P819
2009MNRAS.392..743W