Add to ORKGThe formation and evolution of massive red galaxies form a crucial test of theories of galaxy formation based on hierarchical assembly. In this Letter we use observations of the clustering of luminous red galaxies from the Boötes field and N-body simulations to argue that about of the most luminous satellite galaxies appear to undergo merging or disruption within massive halos between and 0.5
It is a longstanding and remarkable problem when and how red S0 galaxies were formed in clusters of ...
Using galaxy clusters from the ESO Distant Cluster Survey, we study how the distribution of galaxies...
We measure the clustering of extremely red objects (EROs) in 8 deg 2 of the NOAO Deep Wide Field S...
The formation and evolution of massive red galaxies form a crucial test of theories of galaxy format...
We analyze the clustering of red and blue galaxies from four samples spanning a redshift range of 0....
We present an analysis of the small-to-intermediate scale clustering of samples of luminous red gala...
We present predictions for the clustering of Extremely Red Objects (EROs) in a Λ cold dark matter un...
We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by usin...
We trace the assembly history of red galaxies since z=1, by measuring their evolving space density w...
The clustering amplitude of galaxies depends on their intrinsic luminosity. We compare the propertie...
We use measurements of the stellar mass function, galaxy clustering, and galaxy-galaxy lensing withi...
International audienceThe link between massive red galaxies in the local Universe and star-forming g...
We compile a number of observations to estimate the time-averaged rate of formation or buildup of re...
We present an analysis of the small-to-intermediate scale clustering of samples of luminous red gala...
A sample of ~20,000 galaxies covering 0.76 deg2 were observed with the CFHT-UH8K up to V1.4) shows a...
It is a longstanding and remarkable problem when and how red S0 galaxies were formed in clusters of ...
Using galaxy clusters from the ESO Distant Cluster Survey, we study how the distribution of galaxies...
We measure the clustering of extremely red objects (EROs) in 8 deg 2 of the NOAO Deep Wide Field S...
The formation and evolution of massive red galaxies form a crucial test of theories of galaxy format...
We analyze the clustering of red and blue galaxies from four samples spanning a redshift range of 0....
We present an analysis of the small-to-intermediate scale clustering of samples of luminous red gala...
We present predictions for the clustering of Extremely Red Objects (EROs) in a Λ cold dark matter un...
We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by usin...
We trace the assembly history of red galaxies since z=1, by measuring their evolving space density w...
The clustering amplitude of galaxies depends on their intrinsic luminosity. We compare the propertie...
We use measurements of the stellar mass function, galaxy clustering, and galaxy-galaxy lensing withi...
International audienceThe link between massive red galaxies in the local Universe and star-forming g...
We compile a number of observations to estimate the time-averaged rate of formation or buildup of re...
We present an analysis of the small-to-intermediate scale clustering of samples of luminous red gala...
A sample of ~20,000 galaxies covering 0.76 deg2 were observed with the CFHT-UH8K up to V1.4) shows a...
It is a longstanding and remarkable problem when and how red S0 galaxies were formed in clusters of ...
Using galaxy clusters from the ESO Distant Cluster Survey, we study how the distribution of galaxies...
We measure the clustering of extremely red objects (EROs) in 8 deg 2 of the NOAO Deep Wide Field S...