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Optimising the measurement of relativistic distortions in large-scale structure

It has been shown recently that relativistic distortions generate a dipolar modulation in the two-point correlation function of galaxies. To measure this relativistic dipole it is necessary to cross-correlate different populations of galaxies with for example different luminosities or colours. In th...

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Detalles Bibliográficos
Autores principales: Bonvin, Camille, Hui, Lam, Gaztanaga, Enrique
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2016/08/021
http://cds.cern.ch/record/2113299