We investigate the impact of statistical and systematic errors on measurements of linear redshift-space distortions (RSD) in future cosmological surveys by analysing large catalogues of dark matter haloes from the baryonic acoustic oscillation simulations at the Institute for Computational Cosmology. These allow us to estimate the dependence of errors on typical survey properties, as volume, galaxy density and mass (i.e. bias factor) of the adopted tracer. We find that measures of the specific growth rate β = f/b using the Hamilton/Kaiser harmonic expansion of the redshift-space correlation function ξ(rp, π) on scales larger than 3 h−1 Mpc are typically underestimated by up to 10 per cent for galaxy-sized haloes. This is significantly lar...
The anisotropy of clustering in redshift space provides a direct measure of the growth rate of large...
My thesis consists of the two following projects: 1-Testing Large-Scale Structure Measurements ag...
We present measurements of the growth rate of cosmological structure from the modelling of the aniso...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
International audienceRedshift-space distortion (RSD) observed in galaxy redshift surveys is a power...
Redshift-space clustering distortions provide one of the most powerful probes to test the gravity th...
Redshift-space clustering distortions provide one of the most powerful probes to test the gravity th...
We outline how redshift-space distortions (RSD) can be measured from the angular correla-tion functi...
We investigate the use of the cross-correlation between galaxies and galaxy groups to measure redshi...
Measurements of redshift space distortions (RSD) provide a means to test models of gravity on large-...
We investigate the ability of state-of-the-art redshift-space distortion models for the galaxy aniso...
The anisotropy of clustering in redshift space provides a direct measure of the growth rate of large...
My thesis consists of the two following projects: 1-Testing Large-Scale Structure Measurements ag...
We present measurements of the growth rate of cosmological structure from the modelling of the aniso...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
We investigate the impact of statistical and systematic errors on measurements of linear redshift-sp...
International audienceRedshift-space distortion (RSD) observed in galaxy redshift surveys is a power...
Redshift-space clustering distortions provide one of the most powerful probes to test the gravity th...
Redshift-space clustering distortions provide one of the most powerful probes to test the gravity th...
We outline how redshift-space distortions (RSD) can be measured from the angular correla-tion functi...
We investigate the use of the cross-correlation between galaxies and galaxy groups to measure redshi...
Measurements of redshift space distortions (RSD) provide a means to test models of gravity on large-...
We investigate the ability of state-of-the-art redshift-space distortion models for the galaxy aniso...
The anisotropy of clustering in redshift space provides a direct measure of the growth rate of large...
My thesis consists of the two following projects: 1-Testing Large-Scale Structure Measurements ag...
We present measurements of the growth rate of cosmological structure from the modelling of the aniso...