Showing 1–20 of 31 results
/ Date/ Name
Jul 16, 2011BLR Physical Conditions in Extreme Population A Quasars: a Method to Estimate Central Black Hole Mass at High RedshiftNov 18, 2010Physical Conditions in the Broad Line Region of $z\sim3$ Quasars: A Photoionization Method to Derive $r_{BLR}$May 20, 2013Reverberation and photoionization estimates of the Broad Line Region Radius in Low-z QuasarsJul 2, 2025The Lockman-SpReSO project. Spectroscopic analysis of Type 1 AGNAug 4, 2022High Metal Content of Highly Accreting Quasars: Analysis of an Extended SampleFeb 28, 2017Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant UniverseMay 5, 2023SDSS-IV MaNGA: The Incidence of Major Mergers in type I and II AGN Host Galaxies in the DR15 sampleApr 7, 2014A new method to obtain the Broad Line Region size of high redshift quasarsNov 20, 2024An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observationsNov 10, 2014Low- and high-z highly accreting quasars in the 4D Eigenvector 1 contextJan 18, 2023The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-VJun 23, 2014GTC Spectra of z ~ 2.3 Quasars: Comparison with Local Luminosity AnaloguesJan 9, 2024The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxiesMay 6, 2025The eROSITA Final Equatorial Depth Survey (eFEDS): SDSS spectroscopic observations of X-ray sourcesSep 21, 2018Highly accreting quasars: The SDSS low-redshift catalogSep 12, 2025GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxiesApr 28, 2026Spectral Evolution and Transient Broad-Line Features in the Isolated AGN UNAM-KIAS 613Apr 19, 20233D spectroscopy with GTC-MEGARA of the triple AGN candidate in SDSS J102700.40+174900.8May 14, 2007CIV 1549 as an Eigenvector 1 Parameter for Active Galactic NucleiSep 18, 2024The SDSS-V Black Hole Mapper Reverberation Mapping Project: A Kinematically Variable Broad-Line Region and Consequences for Masses of Luminous Quasars