245 citations · 2.2k across the 55 of their papers we have counts for
7 papers · 1 filter
The SFR-radius connection: data and implications for wind strength and halo concentration
Lin Lin, S. M. Faber, David C. Koo +26
This paper is one in a series that explores the importance of radius as a second parameter in galaxy evolution. The topic investigated here is the relationship between star formati…
Quenching as a Contest between Galaxy Halos and their Central Black Holes
Zhu Chen, S. M. Faber, David. C. Koo +27
Existing models of galaxy formation have not yet explained striking correlations between structure and star-formation activity in galaxies, notably the sloped and moving boundaries…
Structural and Stellar Population Properties vs. Bulge Types in Sloan Digital Sky Survey Central Galaxies
Yifei Luo, S. M. Faber, Aldo Rodriguez-Puebla +12
This paper studies pseudo-bulges (P-bulges) and classical bulges (C-bulges) in Sloan Digital Sky Survey central galaxies using the new bulge indicator , which measures relati…
SDSS-IV MaNGA: Effects of Morphology in the global and local Star Formation Main Sequences
M. Cano-Díaz, V. Ávila-Reese, S. F. Sánchez +4
We study the global star-formation rate (SFR) vs. stellar mass (M) correlation, and the spatially-resolved SFR surface density () vs. stellar mass surface density (\Sm…
Astro2020: Empirically Constraining Galaxy Evolution
Peter Behroozi, Matthew R. Becker, Frank C. van den Bosch +22
Over the past decade, empirical constraints on the galaxy-dark matter halo connection have significantly advanced our understanding of galaxy evolution. Past techniques have focuse…
The structural properties of classical bulges and discs from z~2
Paola Dimauro, Marc Huertas-Company, Emanuele Daddi +19
We study the rest-frame optical mass-size relation of bulges and discs from z~2 to z~0 for a complete sample of massive galaxies in the CANDELS fields using 2 component Sérsic mode…
The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
N. Chandrachani Devi, Aldo Rodríguez-Puebla, O. Valenzuela +3
We investigate the dependence of the galaxy-halo connection and galaxy density field in modified gravity models using the body simulations for and nDGP models at .…