Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Compact Molecular Gas Distribution in Quasar Host Galaxies
Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Observational constraints on the structure and evolution of quasars
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Ultraviolet characteristics, outflow properties and variability of active galactic nucleus Markarian 1513
Virial Masses of Black Holes from Single Epoch Spectra of Active Galactic Nuclei
Instrument
HRS, HRS/1, HRS/2, WFPC2, WFPC2/PC
Temporal Coverage
1994-12-29T00:34:17Z/1994-12-29T04:02:17Z
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, HEAP SARA R., 1995, 'IMAGING AND SPECTROSCOPY OF THE NEARBY QSO 2130+099: CYCLE-4 BASELINE', 1.0, European Space Agency, https://doi.org/10.5270/esa-5hyvkjz