Determining Inclinations of Active Galactic Nuclei via their Narrow-line Region Kinematics. I. Observational Results
Dissecting the Power Sources of Low-Luminosity Emission-Line Galaxy Nuclei via Comparison of HST-STIS and Ground-Based Spectra
Optical spectroscopy of local type-1 AGN LINERs
Photoionization Modeling of the Low-luminosity Seyfert 1 Nucleus in NGC 3516
Spatially Resolved Narrow-Line Region Kinematics in Active Galactic Nuclei
The HST view of the broad line region in low luminosity AGN
The HST view of the innermost narrow line region
The supermassive black hole in the Seyfert 2 galaxy NGC 5252
Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
Instrument
STIS, STIS/CCD
Temporal Coverage
1999-01-27T22:48:41Z/2000-06-18T15:06:28Z
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, Macchetto comma F. Duccio, 2001, 'Long Slit Spectroscopy of the Seyfert Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-nggr3p8