Galaxy mass distribution from gravitational light deflection
about
Gravitational Lensing in Astronomy.Modifying gravity: you cannot always get what you want.Cosmology from large-scale galaxy clustering and galaxy–galaxy lensing with Dark Energy Survey Science Verification dataGalaxy–galaxy lensing in the Dark Energy Survey Science Verification dataTruncation of galaxy dark matter halos in high density environmentsGalaxy halo masses and satellite fractions from galaxy-galaxy lensing in the Sloan Digital Sky Survey: stellar mass, luminosity, morphology and environment dependenciesGalaxy bias from galaxy–galaxy lensing in the DES science verification dataPrecision photometric redshift calibration for galaxy–galaxy weak lensingAlgorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clusteringSDSS galaxy bias from halo mass-bias relation and its cosmological implicationsMarginal gravitational lenses of large separation: probing superclustersHow one galaxy can be a cluster
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Galaxy mass distribution from gravitational light deflection
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juni 1984 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в червні 1984
@uk
name
Galaxy mass distribution from gravitational light deflection
@en
Galaxy mass distribution from gravitational light deflection
@nl
type
label
Galaxy mass distribution from gravitational light deflection
@en
Galaxy mass distribution from gravitational light deflection
@nl
prefLabel
Galaxy mass distribution from gravitational light deflection
@en
Galaxy mass distribution from gravitational light deflection
@nl
P2093
P356
P1476
Galaxy mass distribution from gravitational light deflection
@en
P2093
A. P., Jr. Mills
J. A. Tyson
J. F. Jarvis
P356
10.1086/184285
P407
P577
1984-06-01T00:00:00Z