When a galaxy's central supermassive black hole is actively accreting matter, it becomes an active galactic nucleus (AGN). AGN are most commonly found in the "green valley", a region of relatively low density on a color/magnitude diagram of galaxies located between the denser red and blue sequences. I performed an analysis on a sample of galaxies collected from the Sloan Digital Sky Survey (SDSS) database in search of the properties possessed by a target galaxy's neighboring galaxies that correlate with the probability of finding an AGN in that target. I found that, among galaxies with AGN, galaxies with more neighbors – galaxies within a projected distance of 0.5 megaparsecs (Mpc) – tend to be redder than galaxies with few neighbors for th...
International audienceWe explore the dependence of the incidence of moderate-luminosity (L0.5−8 keV ...
191 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2009.We explore how the local envi...
We compare the spatial clustering and physical properties of the active galactic nuclei (AGN) and st...
We analyse the relation between active galactic nuclei (AGN) host properties and large-scale environ...
In this dissertation we study the properties of active galactic nuclei (AGN), which are powered by t...
We present a study of the distribution of AGNs in clusters of galaxies with a uniformly selected, sp...
We have measured the luminous active galactic nucleus (AGN) population in a large sample of clusters...
We present the two-point correlation function (2PCF) of narrow-line active galactic nuclei (AGNs) se...
We study how active galactic nucleus (AGN) activity changes across environments from galaxy pairs to...
Using a large sample of local galaxies (144,940) with-17.5 < Mr <-22 and 0.025 < z < 0.1...
We present evidence that active galactic nuclei (AGN) do not reside in 'special' environments, but i...
The correlation between active galactic nuclei (AGNs) and environment provides important clues to AG...
We present the results of a combined galaxy population analysis for the host galaxies of active gala...
Context. The coeval active galactic nuclei (AGN) and galaxy evolution, and the observed local relati...
We explore the dependence of the incidence of moderate-luminosity (L0.5−8 keV = 1041.9−43.7 erg s-1)...
International audienceWe explore the dependence of the incidence of moderate-luminosity (L0.5−8 keV ...
191 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2009.We explore how the local envi...
We compare the spatial clustering and physical properties of the active galactic nuclei (AGN) and st...
We analyse the relation between active galactic nuclei (AGN) host properties and large-scale environ...
In this dissertation we study the properties of active galactic nuclei (AGN), which are powered by t...
We present a study of the distribution of AGNs in clusters of galaxies with a uniformly selected, sp...
We have measured the luminous active galactic nucleus (AGN) population in a large sample of clusters...
We present the two-point correlation function (2PCF) of narrow-line active galactic nuclei (AGNs) se...
We study how active galactic nucleus (AGN) activity changes across environments from galaxy pairs to...
Using a large sample of local galaxies (144,940) with-17.5 < Mr <-22 and 0.025 < z < 0.1...
We present evidence that active galactic nuclei (AGN) do not reside in 'special' environments, but i...
The correlation between active galactic nuclei (AGNs) and environment provides important clues to AG...
We present the results of a combined galaxy population analysis for the host galaxies of active gala...
Context. The coeval active galactic nuclei (AGN) and galaxy evolution, and the observed local relati...
We explore the dependence of the incidence of moderate-luminosity (L0.5−8 keV = 1041.9−43.7 erg s-1)...
International audienceWe explore the dependence of the incidence of moderate-luminosity (L0.5−8 keV ...
191 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2009.We explore how the local envi...
We compare the spatial clustering and physical properties of the active galactic nuclei (AGN) and st...