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The infrared-radio correlation of spheroid- and disc-dominated star-forming galaxies to z 1.5 in the COSMOS field
Daniel Cs. Molnar, Mark T. Sargent, Jacinta Delhaize +14
Using infrared data from the Herschel Space Observatory and Karl G. Jansky Very Large Array (VLA) 3 GHz observations in the COSMOS field, we investigate the redshift evolution of t…
Dark Galaxy Candidates at Redshift ~3.5 Detected with MUSE
Raffaella Anna Marino, Sebastiano Cantalupo, Simon J. Lilly +18
Recent theoretical models suggest that the early phase of galaxy formation could involve an epoch when galaxies are gas-rich but inefficient at forming stars: a "dark galaxy" phase…
On the evolution of the central density of quiescent galaxies
Sandro Tacchella, C. Marcella Carollo, S. M. Faber +5
We investigate the origin of the evolution of the population-averaged central stellar mass density () of quiescent galaxies (QGs) by probing the relation between stellar age a…
Dust attenuation, bulge formation and inside-out cessation of star-formation in Star-Forming Main Sequence galaxies at z~2
S. Tacchella, C. M. Carollo, N. M. Forster Schreiber +10
We derive two-dimensional dust attenuation maps at resolution from the UV continuum for ten galaxies on the Star-Forming Main Sequence (SFMS). Compari…
Constraints on Quenching of Massive Galaxies from the Evolution of the average Sizes of Star-Forming and Quenched Populations in COSMOS
A. L. Faisst, C. M. Carollo, P. L. Capak +5
We use 9400 quiescent and star-forming galaxies at in COSMOS/UltraVISTA to study the average size evolution of these systems, with focus on t…
Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
R. Genzel, N. M. Förster Schreiber, H. Übler +28
In cold dark matter cosmology, the baryonic components of galaxies are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter, which dominates the t…