A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
A Uniform Analysis of the Lya Forest at z = 0-5. III. Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
A Uniform Analysis of the Lya Forest at z = 0-5. IV. The Clustering and Evolution of Clouds at z <= 1.7
Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
Calibrating C-IV-based Black Hole Mass Estimators
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
Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
Observational constraints on the structure and evolution of quasars
Optical Spectroscopic Atlas of the MOJAVE/2cm AGN Sample
Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei
Instrument
FOS/BL, FOS/RD
Temporal Coverage
1996-03-29T03:12:01Z/1996-08-19T20:57:27Z
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, Eracleous comma Michael, 1997, 'UV SPECTROSCOPY OF RADIO-LOUD AGNS WITH DOUBLE-PEAKED EMISSION LINES', 1.0, European Space Agency, https://doi.org/10.5270/esa-wj8hr5u