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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…
The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients
F. S. Liu, Dongfei Jiang, S. M. Faber +13
The rest-frame UV-optical (i.e., ) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…
Stacking the Cosmic Web in Fluorescent Lyman alpha Emission with MUSE
Sofia G. Gallego, Sebastiano Cantalupo, Simon Lilly +12
Cosmological simulations suggest that most of the matter in the Universe is distributed along filaments connecting galaxies. Illuminated by the cosmic UV background (UVB), these st…
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…
Falling outer rotation curves of star-forming galaxies at 0.6 < z < 2.6 probed with KMOS^3D and SINS/ZC-SINF
P. Lang, N. M. Förster Schreiber, R. Genzel +25
We exploit the deep resolved Halpha kinematic data from the KMOS^3D and SINS/zC-SINF surveys to examine the largely unexplored outer disk kinematics of star-forming galaxies (SFGs)…
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…
Connection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2
Moein Mosleh, Sandro Tacchella, Alvio Renzini +5
We study the history from to of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose we use multi-wa…