Showing 1–20 of 26 results
/ Date/ Name
Oct 2, 2017The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei III: Feedback from Biconical AGN OutflowsSep 13, 2016The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei II: Kinematic Classifications for the Population at z < 0.1Nov 13, 2024DeepUQ: Assessing the Aleatoric Uncertainties from two Deep Learning MethodsAug 25, 2020A Catalog of 406 AGNs in MaNGA: A Connection between Radio-mode AGN and Star Formation QuenchingApr 22, 2024An Excess of AGNs Triggered by Galaxy Mergers in MaNGA Galaxies of Stellar Mass $\sim10^{11}$ $M_{\odot}$Sep 14, 2015The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei I: Very Large Array Detections of Dual AGNs and AGN OutflowsJan 30, 2023A Catalog of 71 Coronal Line Galaxies in MaNGA: [NeV] is an Effective AGN TracerOct 2, 2017An Active Galactic Nucleus Caught in the Act of Turning Off and OnNov 19, 2025Toward Complete Merger Identification at Cosmic Noon with Deep LearningJan 18, 2022Towards a More Complete Optical Census of Active Galactic Nuclei, Via Spatially-Resolved SpectroscopyDec 11, 2023"Beads on a String" Star Formation Tied to one of the most Powerful AGN Outbursts Observed in a Cool Core Galaxy ClusterJul 2, 2019Astro2020 APC White Paper: The Early Career Perspective on the Coming Decade, Astrophysics Career Paths, and the Decadal Survey ProcessOct 26, 2018The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. IV. Association with Galaxy MergersFeb 3, 2020A Second Look at 12 Candidate Dual AGNs using ${\tt BAYMAX}$Mar 27, 2021Evidence of wind signatures in the gas velocity profiles of Red GeysersJan 28, 2021Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST ObservationsApr 19, 2023The First Quiescent Galaxies in TNG300May 5, 2023SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sampleMar 23, 2015Calibrating and Stabilizing Spectropolarimeters with Charge Shuffling and Daytime Sky MeasurementsJul 1, 2025Enhanced Star Formation and Black Hole Accretion Rates in Galaxy Mergers in IllustrisTNG50