Showing 1–20 of 21 results
/ Date/ Name
Mar 16, 2026AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data releaseMay 27, 2019Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatoryAug 10, 2019The Spectral Energy Distributions of Active Galactic NucleiSep 16, 2025VAR-PZ: Constraining the Photometric Redshifts of Quasars using VariabilityAug 31, 2022BASS XXXVII: The role of radiative feedback in the growth and obscuration properties of nearby supermassive black holesSep 2, 2019Photometric redshifts for X-ray-selected active galactic nuclei in the eROSITA eraSep 1, 2021Compton-Thick AGN in the NuSTAR era VI: The observed Compton-thick fraction in the Local UniverseApr 17, 2013The Hubble Space Telescope Treasury Program on the Orion Nebula ClusterJan 21, 2020The Clustering of X-ray Luminous QuasarsJul 25, 2022BASS XXII: The BASS DR2 AGN Catalog and DataJul 14, 2025BASS. XLIX. Characterization of highly luminous and obscured AGNs: local X-ray and [NeV]$λ$3426 emission in comparison with the high-redshift UniverseDec 12, 2019Probing black hole accretion tracks, scaling relations and radiative efficiencies from stacked X-ray active galactic nucleiDec 8, 2020A Large Population of Luminous Active Galactic Nuclei Lacking X-ray Detections: Evidence for Heavy Obscuration?Oct 29, 2020BAT AGN Spectroscopic Survey-XX: Molecular Gas in Nearby Hard X-ray Selected AGN GalaxiesMar 15, 2023A High Fraction of Heavily X-ray Obscured Active Galactic NucleiAug 3, 2023BASS XXXV. The $M_\rm{BH}$-$σ_\rm{\star}$ Relation of 105-Month Swift-BAT Type 1 AGNsJul 25, 2022BAT AGN Spectroscopic Survey XXI: The Data Release 2 OverviewApr 26, 2017X-ray constraints on the fraction of obscured AGN at high accretion luminositiesJan 27, 2025Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within $z < 1.4$ in the Hyper Supreme-Cam Wide SurveyJan 29, 2026Obscured AGN at z < 1.5: X-ray to Far-Infrared SEDs and Host Galaxy Morphologies in the GOODS Fields