Measurements made with the COSMOS machine on deep objective-prism photographs taken with the UK 1.2 m Schmidt Telescope are being used to obtain approximate redshifts (accurate to ≡0.01 in z) for large numbers of galaxies in fields near the South Galactic Pole. The data are suitable for investigations of the distribution of galaxies, such as the detection of large-scale density enhancements or voids
We present the radial velocities and blue, optical magnitudes for all of the galaxies within the Dur...
draft Redshift-Space Distortions (RSD) in galaxy surveys offer a direct route to testing gravity on ...
© 2015, Pleiades Publishing, Inc. A new method for measuring the redshifts of galaxy clusters based ...
A project has been initiated to obtain objective-prism redshifts for large numbers of faint galaxies...
The authors describe a project aimed at determining redshifts for rich clusters of galaxies over a l...
In the last decade much work has been carried out in the development and use of th...
The Muenster Redshift Project (MRSP) is a large low-resolution galaxy-redshift survey, where pairs o...
We present the data from an extensive, moderately deep (bj~9.5) spectroscopic survey of ~ 600 galaxi...
International audienceWe present the results of the ground- and space-based optical and near-infrare...
We present the results of the ground- and space-based optical and near-infrared (NIR) follow-up of 2...
We outline how redshift-space distortions (RSD) can be measured from the angular correla-tion functi...
We present the first results from the Edinburgh-Milano cluster redshift survey. This survey consists...
International audienceWe present a robust approach to estimating the redshift of galaxies using Pan-...
International audienceWe present new results of our wide-field redshift survey of galaxies in a 182 ...
A redshift survey of galaxies located in the direction of the southern Milky Way has been carried ou...
We present the radial velocities and blue, optical magnitudes for all of the galaxies within the Dur...
draft Redshift-Space Distortions (RSD) in galaxy surveys offer a direct route to testing gravity on ...
© 2015, Pleiades Publishing, Inc. A new method for measuring the redshifts of galaxy clusters based ...
A project has been initiated to obtain objective-prism redshifts for large numbers of faint galaxies...
The authors describe a project aimed at determining redshifts for rich clusters of galaxies over a l...
In the last decade much work has been carried out in the development and use of th...
The Muenster Redshift Project (MRSP) is a large low-resolution galaxy-redshift survey, where pairs o...
We present the data from an extensive, moderately deep (bj~9.5) spectroscopic survey of ~ 600 galaxi...
International audienceWe present the results of the ground- and space-based optical and near-infrare...
We present the results of the ground- and space-based optical and near-infrared (NIR) follow-up of 2...
We outline how redshift-space distortions (RSD) can be measured from the angular correla-tion functi...
We present the first results from the Edinburgh-Milano cluster redshift survey. This survey consists...
International audienceWe present a robust approach to estimating the redshift of galaxies using Pan-...
International audienceWe present new results of our wide-field redshift survey of galaxies in a 182 ...
A redshift survey of galaxies located in the direction of the southern Milky Way has been carried ou...
We present the radial velocities and blue, optical magnitudes for all of the galaxies within the Dur...
draft Redshift-Space Distortions (RSD) in galaxy surveys offer a direct route to testing gravity on ...
© 2015, Pleiades Publishing, Inc. A new method for measuring the redshifts of galaxy clusters based ...