none46siAims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the keyparameters that describe the galaxy density field and its spatial correlations in redshift space. Methods. We use the Bayesian formalism to jointly reconstruct the redshift-space galaxy density field, power spectrum, galaxy bias and galaxy luminosity function given the observations and survey selection function. The high-dimensional posterior distribution is explored using the Wiener filter within a Gibbs sampler. We validate the analysis using simulated catalogues and apply it to VIPERS data taking into consideration the inhomogeneous selection function. Results. We present joint constraints on the anisotropic power spectrum, and t...
none37siThe VIPERS galaxy survey has measured the clustering of 0.5 < z < 1.2 galaxies, enabling a n...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
International audienceAims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to ...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims: Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxies (VIPERS...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxi...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxies (VIPERS...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
none50siAims. Building on the two-point correlation function analyses of the VIMOS Public Extragalac...
We use the final catalogue of the VIMOS Public Extragalactic Redshift Survey (VIPERS) to measure the...
20 pages, 15 figuresInternational audienceWe use the first release of the VImos Public Extragalactic...
none37siThe VIPERS galaxy survey has measured the clustering of 0.5 < z < 1.2 galaxies, enabling a n...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
International audienceAims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to ...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims: Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the k...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxies (VIPERS...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxi...
Aims. We use the first release of the VImos Public Extragalactic Redshift Survey of galaxies (VIPERS...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
none50siAims. Building on the two-point correlation function analyses of the VIMOS Public Extragalac...
We use the final catalogue of the VIMOS Public Extragalactic Redshift Survey (VIPERS) to measure the...
20 pages, 15 figuresInternational audienceWe use the first release of the VImos Public Extragalactic...
none37siThe VIPERS galaxy survey has measured the clustering of 0.5 < z < 1.2 galaxies, enabling a n...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...
We compare three methods to measure the count-in-cell probability density function of galaxies in a ...