An irradiated accretion disc in the narrow-line Seyfert 1 RE J1034+396?
A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
Constraining the Black Hole Mass and Accretion Rate in the Narrow-Line Seyfert 1 Galaxy RE J1034+396
Constraining the composition and physics of active galactic nuclei with computer modeling
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
FUSE Observation of the Narrow-Line Seyfert 1 Galaxy RE 1034+39: Dependence of Broad Emission Line Strengths on the Shape of the Photoionizing Spectrum
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
The mass of the black hole in RE J1034+396
The ultraviolet spectrum of the narrow-line Seyfert 1 galaxy RE J1034+396
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Instrument
FOS/BL
Temporal Coverage
1997-01-31T16:26:37Z/1997-01-31T23:02:41Z
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, Puchnarewicz comma Elizabeth M., 1998, 'INVESTIGATING HIGH-TEMPERATURE BIG BUMPS IN AGN', 1.0, European Space Agency, https://doi.org/10.5270/esa-kab9e0t