The evolution of the star-forming interstellar medium across cosmic time
Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …
Physical models of galaxy formation in a cosmological framework
Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …
challenges in astrophysics today due to the vast range of scales and numerous physical …
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty
This work and its companion paper, Amon et al.[Phys. Rev. D 105, 023514 (2022) PRVDAQ
2470-0010 10.1103/PhysRevD. 105.023514], present cosmic shear measurements and …
2470-0010 10.1103/PhysRevD. 105.023514], present cosmic shear measurements and …
A repeating fast radio burst source localized to a nearby spiral galaxy
Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes,. Their physical origin
remains unknown, but dozens of possible models have been postulated. Some FRB sources …
remains unknown, but dozens of possible models have been postulated. Some FRB sources …
First results from the IllustrisTNG simulations: the galaxy colour bimodality
We introduce the first two simulations of the IllustrisTNG project, a next generation of
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …
Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms
ABSTRACT We present Bayesian Analysis of Galaxies for Physical Inference and Parameter
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …
EStimation, or bagpipes, a new python tool that can be used to rapidly generate complex …
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback
In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
3D-HST+ CANDELS: the evolution of the galaxy size–mass distribution since z= 3
A van der Wel, M Franx, PG Van Dokkum… - The Astrophysical …, 2014 - iopscience.iop.org
Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …
3D-HST survey are combined with structural parameter measurements from CANDELS …
The COSMOS2015 galaxy stellar mass function-Thirteen billion years of stellar mass assembly in ten snapshots
We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …
Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses
We have updated the Munich galaxy formation model to the Planck first-year cosmology,
while modifying the treatment of baryonic processes to reproduce recent data on the …
while modifying the treatment of baryonic processes to reproduce recent data on the …