We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) - as defined by the η parameter of Madgwick et al., which quantifies the spectral type of galaxies in the survey. W
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 ga...
We have analysed the distribution of galaxies in groups identified in the largest redshift surveys a...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complica...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
The 2dF Galaxy Redshift Survey (2dFGRS) has already measured over 220,000 redshifts of nearby (z ~0....
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
Spectroscopic redshift surveys can map the spatial distribution of galaxy samples. They can be used ...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complica...
We calculate the optical b (J) luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) f...
The 2dF Galaxy Redshift Survey (2dFGRS) of 230,000 redshifts of nearby (z~0.1) galaxies is now compl...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Gal...
We have calculated the two-point correlation functions in redshift space, Ζ (σ, π), for galaxies of ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 ga...
We have analysed the distribution of galaxies in groups identified in the largest redshift surveys a...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complica...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
The 2dF Galaxy Redshift Survey (2dFGRS) has already measured over 220,000 redshifts of nearby (z ~0....
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias ...
Spectroscopic redshift surveys can map the spatial distribution of galaxy samples. They can be used ...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complica...
We calculate the optical b (J) luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) f...
The 2dF Galaxy Redshift Survey (2dFGRS) of 230,000 redshifts of nearby (z~0.1) galaxies is now compl...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Gal...
We have calculated the two-point correlation functions in redshift space, Ζ (σ, π), for galaxies of ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 ga...
We have analysed the distribution of galaxies in groups identified in the largest redshift surveys a...