Add to ORKGThe goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ∼1.7 deg2 in the COSMOS field. Galaxies have been divided according to their star formation activity and the evolution of the different populations, in particular of the quiescent galaxies, has been investigated in detail. We have studied an IRAC (mag 3.6 μm 2.5 (logρ[M⊙ Mpc−3]∼ 6), meaning that efficient star formation had to take place before that tim
We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to tr...
We combine high-resolution Hubble Space Telescope/WFC3 images with multi- wavelength photometry to t...
International audienceWe aim to measure the average dust and molecular gas content of massive star-f...
The goal of this work is to study the evolution of high-redshift (z ≥ 1.4) quiescent galaxies over a...
The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an...
The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an...
Aims. Questions of how massive quiescent galaxies rapidly assembled and how abundant they are at hig...
We present a sample of 151 massive (M∗ > 1010 M·) quiescent galaxies at 2 < z < 5, based on...
With a complete, mass-selected sample of quiescent galaxies from the NEWFIRM Medium-Band Survey, we ...
We present star formation histories (SFHs) for a sample of 104 massive (stellar mass M > 10^10 M_⊙) ...
We report on the spectroscopic confirmation of a massive quiescent galaxy at $z_\mathrm{spec}=4.53$ ...
none4noThe presence of massive quiescent galaxies at high redshifts is still a challenge for most mo...
V. W. and K. R. acknowledge support of the European Research Council via the award of a starting gra...
Although there has been much progress in understanding how galaxies evolve, we still do not understa...
We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to tr...
We combine high-resolution Hubble Space Telescope/WFC3 images with multi- wavelength photometry to t...
International audienceWe aim to measure the average dust and molecular gas content of massive star-f...
The goal of this work is to study the evolution of high-redshift (z ≥ 1.4) quiescent galaxies over a...
The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an...
The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an...
Aims. Questions of how massive quiescent galaxies rapidly assembled and how abundant they are at hig...
We present a sample of 151 massive (M∗ > 1010 M·) quiescent galaxies at 2 < z < 5, based on...
With a complete, mass-selected sample of quiescent galaxies from the NEWFIRM Medium-Band Survey, we ...
We present star formation histories (SFHs) for a sample of 104 massive (stellar mass M > 10^10 M_⊙) ...
We report on the spectroscopic confirmation of a massive quiescent galaxy at $z_\mathrm{spec}=4.53$ ...
none4noThe presence of massive quiescent galaxies at high redshifts is still a challenge for most mo...
V. W. and K. R. acknowledge support of the European Research Council via the award of a starting gra...
Although there has been much progress in understanding how galaxies evolve, we still do not understa...
We combine high-resolution Hubble Space Telescope/WFC3 images with multi-wavelength photometry to tr...
We combine high-resolution Hubble Space Telescope/WFC3 images with multi- wavelength photometry to t...
International audienceWe aim to measure the average dust and molecular gas content of massive star-f...