A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Estimating Black Hole Masses in Active Galactic Nuclei Using the Mg II l2800 Emission Line
Evolution of the Outflows in NGC 3516
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
Intrinsic absorption with the Far Ultraviolet Spectroscopic Explorer
NGC 3516: The Long-Term Variability of the Active Galactic Nucleus Emission-Line and Absorption-Line Regions
Observational constraints on the structure and evolution of quasars
On the Absence of Broad Mg II Emission Line Variability in NGC 3516 during 1996
Strong Correlation between Fe II/Mg II Ratio and Eddington Ratio of Type 1 Active Galactic Nuclei
Variable Ultraviolet Absorption in the Seyfert 1 Galaxy NGC 3516: The Case for Associated Ultraviolet and X-Ray Absorption
Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei
Instrument
FOS/BL, FOS/RD
Temporal Coverage
1995-12-30T02:29:56Z/1996-11-28T03:19:12Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Koratkar et al., 1997, 'NGC 3516: A Critical Test-case for AGN Absorption and Emission Line Regions', 1.0, European Space Agency, https://doi.org/10.5270/esa-9v22mxe
