BAL outflow in quasar B0254-3327B: analysis and comparison with other extreme UV outflows
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Estimating Black Hole Masses in Active Galactic Nuclei Using the Mg II l2800 Emission Line
Evidence of the Dynamics of Relativistic Jet Launching in Quasars
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Low Redshift BAL QSOs in the Eigenvector 1 Context
Supermassive Black Hole Mass Estimates Using Sloan Digital Sky Survey Quasar Spectra at 0.7 < z < 2
The Chemical Properties of Low-redshift QSOs
The influence of gravitational lensing on the spectra of lensed quasi-stellar objects
The Optical and Ultraviolet Emission-line Properties of Bright Quasars with Detailed Spectral Energy Distributions
The Properties and Evolution of the Highly Ionized Gas in MR 2251-178
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Ultraviolet Structure in the Lensed QSO 0957+561
Variability of Narrow, Associated Absorption Lines in Moderate- and Low-Redshift Quasars
Variable Ultraviolet Absorption in the Spectrum of MR 2251-178
Weighing supermassive black holes
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2000-09-08T06:30:19Z/2001-08-18T12:53:33Z
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, Charlton comma Jane C., 2002, 'A Snapshot Survey of Variability of Narrow and Broad Associated Absorption Lines in Quasars', 1.0, European Space Agency, https://doi.org/10.5270/esa-9j6m2c7