We find a significant number of massive and compact galaxies in clusters from the ESO Distant Clusters Survey (EDisCS) at 0.4 4 x 10(11) M-circle dot have significantly increased by a factor of 2 and 4, respectively, confirming the results of a number of recent works on the subject. Our findings show that progenitor bias effects play an important role in the size-growth paradigm of massive and passive galaxies
We present evidence for a strong relationship between galaxy size and environment for the quiescent ...
In order to assess whether the environment has a significant effect on galaxy sizes, we compare the ...
International audience(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically c...
We find a significant number of massive and compact galaxies in clusters from the ESO Distant Cluste...
We find a significant number of massive and compact galaxies in clusters from the ESO Distant Cluste...
Most massive galaxies are compact at high redshifts, but similarly compact massive galaxies are rare...
Most massive passive galaxies are compact at high redshifts, but similarly compact massive galaxies ...
International audienceWe analyse the mass-size relation of ∼400 quiescent massive ETGs (M * /M > 3 ×...
We analyse the mass–size relation of ∼400 quiescent massive ETGs (M*/M⊙ > 3 × 1010) hosted by mas...
Massive quiescent galaxies at z > 1 have been found to have small physical sizes, and hence to be...
International audienceThe mass and structural evolution of massive galaxies is one of the hottest to...
We present the size-luminosity relation (SLR) for disk galaxies observed in eight clusters from the ...
We present evidence for a strong relationship between galaxy size and environment for the quiescent ...
International audienceWe set out to quantify the number density of quiescent massive compact galaxie...
We study the evolution of spectral early-type galaxies in clusters, groups, and the field up to reds...
We present evidence for a strong relationship between galaxy size and environment for the quiescent ...
In order to assess whether the environment has a significant effect on galaxy sizes, we compare the ...
International audience(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically c...
We find a significant number of massive and compact galaxies in clusters from the ESO Distant Cluste...
We find a significant number of massive and compact galaxies in clusters from the ESO Distant Cluste...
Most massive galaxies are compact at high redshifts, but similarly compact massive galaxies are rare...
Most massive passive galaxies are compact at high redshifts, but similarly compact massive galaxies ...
International audienceWe analyse the mass-size relation of ∼400 quiescent massive ETGs (M * /M > 3 ×...
We analyse the mass–size relation of ∼400 quiescent massive ETGs (M*/M⊙ > 3 × 1010) hosted by mas...
Massive quiescent galaxies at z > 1 have been found to have small physical sizes, and hence to be...
International audienceThe mass and structural evolution of massive galaxies is one of the hottest to...
We present the size-luminosity relation (SLR) for disk galaxies observed in eight clusters from the ...
We present evidence for a strong relationship between galaxy size and environment for the quiescent ...
International audienceWe set out to quantify the number density of quiescent massive compact galaxie...
We study the evolution of spectral early-type galaxies in clusters, groups, and the field up to reds...
We present evidence for a strong relationship between galaxy size and environment for the quiescent ...
In order to assess whether the environment has a significant effect on galaxy sizes, we compare the ...
International audience(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically c...