activity
19942023
most citedThe Demography of Massive Dark Objects in Galaxy Centres

4k citations · 49.5k across the 249 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.CO2010★ 29 cited

Automated Morphological Classification of SDSS Red Sequence Galaxies

Judy Y. Cheng, S. M. Faber, Luc Simard +4

(abridged) In the last decade, the advent of enormous galaxy surveys has motivated the development of automated morphological classification schemes to deal with large data volumes…

astro-ph.CO2010★ 30 cited

Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories

Genevieve J. Graves, S. M. Faber, Ricardo P. Schiavon

In the three-dimensional parameter space defined by velocity dispersion, effective radius (R_e), and effective surface brightness (I_e), early-type galaxies are observed to populat…

astro-ph.CO2010★ 80 cited

Absence of Evidence Is Not Evidence of Absence: The Color-Density Relation at Fixed Stellar Mass Persists to z ~ 1

Michael C. Cooper, Alison L. Coil, Brian F. Gerke +12

We use data drawn from the DEEP2 Galaxy Redshift Survey to investigate the relationship between local galaxy density, stellar mass, and rest-frame galaxy color. At z ~ 0.9, we find…

astro-ph.CO2010★ 101 cited

AEGIS: Demographics of X-ray and Optically Selected AGNs

Renbin Yan, Luis C. Ho, Jeffrey A. Newman +19

We develop a new diagnostic method to classify galaxies into AGN hosts, star-forming galaxies, and absorption-dominated galaxies by combining the [O III]/Hbeta ratio with rest-fram…

astro-ph.CO2010★ 710 cited

Extragalactic Background Light Inferred from AEGIS Galaxy SED-type Fractions

A. Dominguez, J. R. Primack, D. J. Rosario +15

The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for gamma-ray astronomy, but the overall spe…

astro-ph.CO2010★ 113 cited

Dissecting the Red Sequence - III. Mass-to-Light Variations in 3D Fundamental Plane Space

Genevieve J. Graves, S. M. Faber

The Fundamental Plane has finite thickness and is tilted from the virial relation, indicating that dynamical mass-to-light ratios (Mdyn/L) vary among early type galaxies. We use a…