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
Below the Lyman Edge: Ultraviolet Polarimetry of Quasars
Do All the Quasars and High-excitation Radio Galaxies (HERGs) in the 3CRR Catalog Contain a Magnetically Arrested Disk (MAD)?
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Evidence of the Dynamics of Relativistic Jet Launching in Quasars
Low- and High-Ionization Absorption Properties of Mg II Absorption-selected Galaxies at Intermediate Redshifts. I. General Properties
Models of Five Absorption-Line Systems along the Line of Sight Toward PG 0117+213
The Population of Weak Mg II Absorbers. II. The Properties of Single-Cloud Systems
Instrument
FOS/BL
Temporal Coverage
1996-02-12T22:54:09Z/1996-03-24T01:20:27Z
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, Koratkar comma Anuradha P., 1997, 'Spectropolarimetry of Low Red-Shift Quasars - Test of the Emission Mechanism', 1.0, European Space Agency, https://doi.org/10.5270/esa-k3awc36
