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Lusso, E.Treister, Ezequiel.Hennawi, J. F.Comastri, A.Zamorani, G.Richards, G. T.Vignali, C.Schawinski, KevinSalvato, M.Gilli, R.[The Obscured Fraction of Active Galactic Nuclei in the XMM-COSMOS Survey: A Spectral Energy Distribution Perspective]The Obscured Fraction of Active Galactic Nuclei in the XMM-COSMOS Survey: A Spectral Energy Distribution Perspective

Treister, Ezequiel.Schawinski, KevinVolonteri, MartaNatarajan, Priyamvada[New observational constraints on the growth of the First Supermassive Black Holes.]New observational constraints on the growth of the First Supermassive Black Holes.

Teng, Stacy H.Treister, Ezequiel.Schawinski, KevinUrry, C. MegDarg, Dan W.Kaviraj, SugataOh, KyuseokBonning, Erin W.Cardamone, Carolin N.Keel, William C.Lintott, Chris J.Simmons, Brooke D.[Chandra Observations of Galaxy Zoo Mergers : Frequency of Binary Active Nuclei in Massive Mergers.]Chandra Observations of Galaxy Zoo Mergers : Frequency of Binary Active Nuclei in Massive Mergers.

Treister, Ezequiel.Schawinski, KevinUrry, C. MegSimmons, Brooke D.[Major Galaxy Mergers Only Trigger the Most Luminous Active Galactic Nuclei.]Major Galaxy Mergers Only Trigger the Most Luminous Active Galactic Nuclei.

Schawinski, KevinTreister, Ezequiel.Simmons, Brooke D.Urry, C. MegGlikman, Eilat[Heavily obscured quasar host galaxies at z ∼ 2 are discs, not major mergers.]Heavily obscured quasar host galaxies at z ∼ 2 are discs, not major mergers.

Koss, M.Ricci, ClaudioTreister, Ezequiel.Trakhtenbrot, BennyLamperti, IsabellaOh, KyuseokBerney, SimonSchawinski, KevinBaloković, MislavBaronchelli, LindaCrenshaw, D. Michael[BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics.]BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics.

Ricci, ClaudioTreister, Ezequiel.Trakhtenbrot, BennyKoss, M.Ueda, YoshihiroSchawinski, KevinOh, KyuseokLamperti, IsabellaMushotzky, RichardHo, Luis C.Weigel, Anna K.[The close environments of accreting massive black holes are shaped by radiative feedback.]The close environments of accreting massive black holes are shaped by radiative feedback.

Olivares, V.Treister, Ezequiel.Privon, George C.Alaghband-Zadeh, S.Casey, Caitlin M.Schawinski, KevinKurczynski, PeterGawiser, Eric.Nagar, NeilChapman, S.Bauer, Franz Erik.[Spatially Resolved Spectroscopy of Submillimeter Galaxies at z ≃ 2]Spatially Resolved Spectroscopy of Submillimeter Galaxies at z ≃ 2

Sartori, Lia F.Schawinski, KevinKoss, M.Treister, Ezequiel.Maksym, W. PeterKeel, William C.Urry, C. MeganLintott, Chris J.Wong, O. Ivy[Extended X-ray emission in the IC 2497 - Hanny's Voorwerp system: energy injection in the gas around a fading AGN.]Extended X-ray emission in the IC 2497 - Hanny's Voorwerp system: energy injection in the gas around a fading AGN.

Sartori, Lia F.Treister, Ezequiel.Schawinski, KevinTrakhtenbrot, BennyKoss, M.Shirazi, MaryamOh, Kyuseok[The search for active black holes in nearby low-mass galaxies using optical and mid-IR data.]The search for active black holes in nearby low-mass galaxies using optical and mid-IR data.

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