A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Feedback from Mass Outflows in Nearby Active Galactic Nuclei. I. Ultraviolet and X-Ray Absorbers
GHRS Monitoring of the Outflowing Material in NGC 4151
Goddard High Resolution Spectrograph Observations of NGC 4151
Intrinsic Absorption Lines in Seyfert 1 Galaxies. I. Ultraviolet Spectra from the Hubble Space Telescope
O VI, N V, and C IV in the Galactic Halo. II. Velocity-Resolved Observations with the Hubble Space Telescope and Far Ultraviolet Spectroscopic Explorer
Probing the Ionization Structure of the Narrow-Line Region in the Seyfert 1 Galaxy NGC 4151
Simultaneous Ultraviolet and X-Ray Observations of the Seyfert Galaxy NGC 4151. II. Physical Conditions in the UV Absorbers
Space Telescope Imaging Spectrograph Echelle Observations of the Seyfert Galaxy NGC 4151: Physical Conditions in the Ultraviolet Absorbers
Instrument
FOS/BL, HRS, HRS/2
Temporal Coverage
1994-10-28T22:20:11Z/1996-03-11T20:50:16Z
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, Weymann et al., 1997, 'HIGH RES SPECT OF THE NUCLEUS OF NGC 4151: CYCLE 4, HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-8kb5x3x
