activity
20122025
most citedA Link Between Star Formation Quenching and Inner Stellar Mass Density in SDSS Central Galaxies

311 citations · 2.2k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2025

Tracing Quenching in Nearby Galaxies Through Inner Surface Mass Density and Cold Gas Content

Evangela E. Shread, Trevor J. Weiss, Jerome J. Fang +1

The inner stellar mass surface density within 1 kpc, Sigma1, has emerged as a suitable proxy for bulge growth and galaxy quenching. However, the dependence of cold gas content on S…

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.GA2019★ 18 cited

Deep ugrizY Imaging and DEEP2/3 Spectroscopy: A Photometric Redshift Testbed for LSST and Public Release of Data from the DEEP3 Galaxy Redshift Survey

Rongpu Zhou, Michael C. Cooper, Jeffrey A. Newman +19

We present catalogs of calibrated photometry and spectroscopic redshifts in the Extended Groth Strip, intended for studies of photometric redshifts (photo-z's). The data includes u…

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.GA2018★ 21 cited

On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS

F. S. Liu, Meng Jia, Hassen M. Yesuf +19

We investigate the galaxy quenching process at intermediate redshift using a sample of galaxies with between redshift 0.5 and 1.0 in all fiv…

astro-ph.GA2018★ 7 cited

The Isophotal Structure of Star-forming Galaxies at in CANDELS: Implications for the Evolution of Galaxy Structure

Dongfei Jiang, F. S. Liu, Xianzhong Zheng +15

We have measured the radial profiles of isophotal ellipticity () and disky/boxy parameter A out to radii of about three times the semi-major axes for s…

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★ 27 cited

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…

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…

astro-ph.GA2016★ 91 cited

The Nature of Massive Transition Galaxies in CANDELS, GAMA, and Cosmological Simulations

Viraj Pandya, Ryan Brennan, Rachel S. Somerville +25

We explore observational and theoretical constraints on how galaxies might transition between the "star-forming main sequence" (SFMS) and varying "degrees of quiescence" out to $z=…

astro-ph.GA2016★ 39 cited

The UV-optical Color Gradients in Star-Forming Galaxies at 0.5<z<1.5: Origins and Link to Galaxy Assembly

F. S. Liu, Dongfei Jiang, Yicheng Guo +10

The rest-frame UV-optical (i.e., NUV-B) color index is sensitive to the low-level recent star formation and dust extinction, but it is insensitive to the metallicity. In this Lette…

astro-ph.GA2015★ 265 cited

A universal structural and star-forming relation since : connecting compact star-forming and quiescent galaxies

G. Barro, S. M. Faber, D. C. Koo +13

We study the evolution of the core (r<1 kpc) and effective (r<r_e) stellar-mass surface densities, in star-forming and quiescent galaxies. Since z=3, both populations occupy distin…

astro-ph.GA2015★ 44 cited

Caught in the act: gas and stellar velocity dispersions in a fast quenching compact star-forming galaxy at z~1.7

G. Barro, S. M. Faber, A. Dekel +20

We present Keck-I MOSFIRE spectroscopy in the Y and H bands of GDN-8231, a massive, compact, star-forming galaxy (SFG) at a redshift . Its spectrum reveals both H and…

astro-ph.GA2014★ 241 cited

Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Yicheng Guo, Henry C. Ferguson, Eric F. Bell +19

Although giant clumps of stars are crucial to galaxy formation and evolution, the most basic demographics of clumps are still uncertain, mainly because the definition of clumps has…

astro-ph.GA2014★ 71 cited

Galaxy Zoo: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2 < z < 1.0?

Edmond Cheung, Jonathan R. Trump, E. Athanassoula +19

We present a new study investigating whether active galactic nuclei (AGN) beyond the local universe are preferentially fed via large-scale bars. Our investigation combines data fro…

astro-ph.GA2014★ 45 cited

Reverberation Mapping of the Kepler-Field AGN KA1858+4850

Liuyi Pei, Aaron J. Barth, Greg S. Aldering +40

KA1858+4850 is a narrow-line Seyfert 1 galaxy at redshift 0.078 and is among the brightest active galaxies monitored by the Kepler mission. We have carried out a reverberation mapp…

astro-ph.GA2014★ 112 cited

From Starburst to Quiescence: Testing AGN feedback in Rapidly Quenching Post-Starburst Galaxies

Hassen M. Yesuf, S. M. Faber, Jonathan R. Trump +5

Post-starbursts are galaxies in transition from the blue cloud to the red sequence. Although they are rare today, integrated over time they may be an important pathway to the red s…

astro-ph.GA2014★ 89 cited

Keck-I MOSFIRE spectroscopy of compact star-forming galaxies at z2: High velocity dispersions in progenitors of compact quiescent galaxies

G. Barro, J. R. Trump, D. C. Koo +28

We present Keck-I MOSFIRE near-infrared spectroscopy for a sample of 13 compact star-forming galaxies (SFGs) at redshift with star formation rates of SFR100…

astro-ph.CO2013★ 311 cited

A Link Between Star Formation Quenching and Inner Stellar Mass Density in SDSS Central Galaxies

Jerome J. Fang, S. M. Faber, David C. Koo +1

We study the correlation between galaxy structure and the quenching of star formation using a sample of SDSS central galaxies with stellar masses 9.75< log M_*/M_sun<11.25 and reds…

astro-ph.CO2012★ 39 cited

A Census of Broad-Line Active Galactic Nuclei in Nearby Galaxies: Coeval Star Formation and Rapid Black Hole Growth

Jonathan R. Trump, Alexander D. Hsu, Jerome J. Fang +3

We present the first quantified, statistical map of broad-line active galactic nucleus (AGN) frequency with host galaxy color and stellar mass in nearby (0.01 < z < 0.11) galaxies.…

astro-ph.GA2012★ 242 cited

The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey

Edmond Cheung, S. M. Faber, David C. Koo +25

The shutdown of star formation in galaxies is generally termed `quenching'. Although quenching may occur through a variety of processes, the exact mechanism(s) that is in fact resp…

astro-ph.CO2012★ 73 cited

The Slow Death (or Rebirth?) of Extended Star Formation in z~0.1 Green Valley Early-Type Galaxies

Jerome J. Fang, S. M. Faber, Samir Salim +2

UV observations in the local universe have uncovered a population of early-type galaxies with UV flux consistent with low-level recent or ongoing star formation. We present resolve…