Showing 1–19 of 19 results
/ Date/ Name
Dec 20, 2004What is the origin of the soft excess in AGN?Mar 20, 2014Stochastic Modeling of the Fermi/LAT Gamma-ray Blazar VariabilitySep 8, 2006What is the origin of the soft excess in AGN?May 17, 2017The origin of the Ultraluminous X-ray SourcesFeb 3, 2011Simulated spectral states of AGN and observational predictionsMar 30, 2015Nature of the Extreme Ultraluminous X-ray SourcesJan 15, 2009What can we learn about quasars from alpha_OX measurements in galactic black hole binaries?Apr 7, 2016First detection in gamma-rays of a young radio galaxy: Fermi-LAT observations of the Compact Symmetric Object PKS 1718-649Jun 26, 2024Active Galaxy Science with the Line Emission Mapper: The Case for High-Resolution Soft X-ray SpectroscopyNov 4, 2021The Origin of High Energy Emission in the Young Radio Source PKS 1718-649Sep 29, 2010A Stochastic Model for the Luminosity Fluctuations of Accreting Black HolesNov 3, 2006Evolution of the X-ray Emission of Radio-Quiet QuasarsAug 3, 2025Using Faded Changing-Look Quasars to Unveil the Spectral Energy Distribution Evolution of Low-Luminosity Active Galactic NucleiJun 8, 2011Evidence for a change in the X-ray radiation mechanism in the hard state of Galactic black holesAug 22, 2012Nuclear X-ray properties of the peculiar radio-loud hidden AGN 4C+29.30Dec 5, 2018The Impact of the Environment on the Early Stages of Radio Source EvolutionOct 7, 2004High redshift radio quiet quasars -- exploring parameter space of accretion models. Part II: patchy corona modelSep 4, 2019First Hard X-ray Observation of a Compact Symmetric Object: A Broadband X-ray Study of a radio galaxy OQ+208 with NuSTAR and ChandraOct 7, 2004High redshift radio quiet quasars - exploring the parameter space of accretion models. Part I: hot semi-spherical flow