A Complete Atlas of Recalibrated Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars. I. Pre-COSTAR Spectra
Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
Broad Emission Line Variability as a Constraint upon the Physical Conditions within the Broad Emission Line Region of NGC 5548
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Comparative Analysis of the High- and Low-Ionization Lines in the Broad-Line Region of Active Galactic Nuclei
Deep Optical Imaging of the Bright Seyfert Galaxy NGC 5548: A Long, Very Low Surface Brightness Tail
Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
Dynamics of Broad Emission-Line Region in NGC 5548: Hydromagnetic Wind Model versus Observations
Estimating reddening of the continuum and broad-line region of active galactic nuclei: the mean reddening of NGC 5548 and the size of the accretion disc
In Situ Star Formation in Accretion Disks and Explanation of Correlation between the Black Hole Mass and Metallicity in Active Galactic Nuclei
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
Keplerian Motion of Broad-Line Region Gas as Evidence for Supermassive Black Holes in Active Galactic Nuclei
Locally Optimally Emitting Clouds and the Variable Broad Emission Line Spectrum of NGC 5548
Observations of O I and Ca II Emission Lines in Quasars: Implications for the Site of Fe II Line Emission
Outflows from active galactic nuclei: the BLR-NLR metallicity correlation
Quantifying the impact of variable BLR diffuse continuum contributions on measured continuum interband delays
Simultaneous Ultraviolet and X-Ray Spectroscopy of the Seyfert 1 Galaxy NGC 5548. I. Physical Conditions in the Ultraviolet Absorbers
Space Telescope and Optical Reverberation Mapping Project. IV. Anomalous Behavior of the Broad Ultraviolet Emission Lines in NGC 5548
Steps toward Determination of the Size and Structure of the Broad-Line Region in Active Galactic Nuclei. VIII. an Intensive HST, IUE, and Ground-based Study of NGC 5548
The Geometry and Kinematics of the Broad-Line Region in NGC 5548 from HST and IUE Observations
The Redshifted Excess in Quasar C IV Broad Emission Lines
The Ultraviolet-Optical Albedo of Broad Emission Line Clouds
The Variable Diffuse Continuum Emission of Broad-Line Clouds
Variability of Fe II Emission Features in the Seyfert 1 Galaxy NGC 5548
Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei
Instrument
FOS/BL
Temporal Coverage
1993-04-19T09:41:04Z/1993-05-27T15:25:41Z
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, Peterson comma Bradley M, 1994, 'PROBING THE NUCLEAR REGIONS OF THE SEYFERT GALAXY NGC 5548 - CONTINUATION', 1.0, European Space Agency, https://doi.org/10.5270/esa-w243i42