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4 papers · 2 filters
Do We Expect Most AGN to Live in Disks?
Philip F. Hopkins, Dale D. Kocevski, Kevin Bundy
Recent observations have indicated that a large fraction of the low to intermediate luminosity AGN population lives in disk-dominated hosts, while the more luminous quasars live in…
Evolution of the Stellar-to-Dark Matter Relation: Separating Star-Forming and Passive Galaxies from z=1 to 0
Jeremy L. Tinker, Alexie Leauthaud, Kevin Bundy +5
We use measurements of the stellar mass function, galaxy clustering, and galaxy-galaxy lensing within the COSMOS survey to constrain the stellar-to-halo mass relation (SHMR) of sta…
Evolution of Galaxies and their Environments at z = 0.1 to 3 in COSMOS
N. Scoville, S. Arnouts, H. Aussel +43
Large-scale structures (LSS) out to z are measured in the Cosmic Evolution Survey (COSMOS) using extremely accurate photometric redshifts (photoz). The Ks-band selected sam…
Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
Matthew R. George, Chung-Pei Ma, Kevin Bundy +5
While the star formation rates and morphologies of galaxies have long been known to correlate with their local environment, the process by which these correlations are generated is…