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20132022
most citedQuenching as a Contest between Galaxy Halos and their Central Black Holes

108 citations · 509 across the 13 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2021★ 12 cited

Implications of Increased Central Mass Surface Densities for the Quenching of Low-mass Galaxies

Yicheng Guo, Timothy Carleton, Eric F. Bell +12

We use the Cosmic Assembly Deep Near-infrared Extragalactic Legacy Survey (CANDELS) data to study the relationship between quenching and the stellar mass surface density within the…

astro-ph.GA2019★ 12 cited

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…

astro-ph.GA2019★ 108 cited

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…

astro-ph.GA2019★ 35 cited

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…

astro-ph.GA2018★ 24 cited

Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts

Weichen Wang, Susan A. Kassin, Camilla Pacifici +11

At intermediate and high redshifts, measurements of galaxy star-formation rates are usually based on rest-frame ultraviolet (UV) data. A correction for dust attenuation, A_UV, is n…

astro-ph.GA2018★ 73 cited

The evolution of galaxy shapes in CANDELS: from prolate to oblate

Haowen Zhang, Joel R. Primack, S. M. Faber +9

We model the projected b/a-log a distributions of CANDELS main sequence star-forming galaxies, where a (b) is the semi-major (semi-minor) axis of the galaxy images. We find that sm…

astro-ph.GA2017★ 102 cited

Demographics of Star-forming Galaxies since . I. The Diagram in CANDELS

Jerome J. Fang, S. M. Faber, David C. Koo +41

This is the first in a series of papers examining the demographics of star-forming galaxies at in CANDELS. We study 9,100 galaxies from GOODS-S and UDS having published…

astro-ph.GA2017★ 35 cited

CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies

Yicheng Guo, Eric F. Bell, Yu Lu +17

We investigate the environmental quenching of galaxies, especially those with stellar masses (M*), beyond the local universe. Essentially all local low-mass quen…

astro-ph.GA2017★ 55 cited

UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles

Weichen Wang, S. M. Faber, F. S. Liu +10

This paper uses radial colour profiles to infer the distributions of dust, gas and star formation in z=0.4-1.4 star-forming main sequence galaxies. We start with the standard UVJ-b…