We introduce a simple linear equation relating the line-of-sight peculiar-velocity and density contrast correlation functions. The relation, which we call the Gaussian cell two-point 'energy-like' equation, is valid at the distant-observer limit and requires Gaussian smoothed fields. In the variance case, i.e. at zero lag, the equation is similar in its mathematical form to the Irvine-Layzer cosmic energy equation. beta estimation with this equation from the Point Source Catalogue Redshift (PSC) survey and the SEcat catalogue of peculiar velocities is carried out, returning a value of beta = 0.44 +/- 0.08. The applicability of the method for the 6dF galaxy redshift and peculiar motions survey is demonstrated with mock data where it is shown...
We estimate the mass density fluctuations power spectrum (PS) on large scales by applying a maximum ...
We report on the measurement of the two-point correlation function and the pairwise peculiar velocit...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We introduce a simple linear equation relating the line-of-sight peculiar-velocity and density contr...
We introduce a simple linear equation relating the line-of-sight peculiar-velocity and density contr...
We introduce a simple linear equation relating the line-of-sight peculiar velocity and density contr...
This thesis focuses on constraining the linear redshift distortion parameter β, which is a critical ...
Given a redshift survey of galaxies with measurements of apparent magnitudes, we present a novel met...
We introduce a new estimator of the peculiar velocity of a galaxy or group of galaxies from redshift...
We present scale-dependent measurements of the normalized growth rate of structure fσ8(k, z = 0) usi...
The growth history of large-scale structure in the Universe is a powerful probe of the cosmological ...
To understand the nature of the accelerated expansion of the Universe, we need to combine constraint...
Low redshift surveys of galaxy peculiar velocities provide a wealth of cosmological information. We ...
Peculiar velocity surveys, which measure galaxy velocities directly from standard candles in additio...
The distribution of angles subtended between pairs of galaxies and the line of sight, which is unifo...
We estimate the mass density fluctuations power spectrum (PS) on large scales by applying a maximum ...
We report on the measurement of the two-point correlation function and the pairwise peculiar velocit...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We introduce a simple linear equation relating the line-of-sight peculiar-velocity and density contr...
We introduce a simple linear equation relating the line-of-sight peculiar-velocity and density contr...
We introduce a simple linear equation relating the line-of-sight peculiar velocity and density contr...
This thesis focuses on constraining the linear redshift distortion parameter β, which is a critical ...
Given a redshift survey of galaxies with measurements of apparent magnitudes, we present a novel met...
We introduce a new estimator of the peculiar velocity of a galaxy or group of galaxies from redshift...
We present scale-dependent measurements of the normalized growth rate of structure fσ8(k, z = 0) usi...
The growth history of large-scale structure in the Universe is a powerful probe of the cosmological ...
To understand the nature of the accelerated expansion of the Universe, we need to combine constraint...
Low redshift surveys of galaxy peculiar velocities provide a wealth of cosmological information. We ...
Peculiar velocity surveys, which measure galaxy velocities directly from standard candles in additio...
The distribution of angles subtended between pairs of galaxies and the line of sight, which is unifo...
We estimate the mass density fluctuations power spectrum (PS) on large scales by applying a maximum ...
We report on the measurement of the two-point correlation function and the pairwise peculiar velocit...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...