A Comparison between the Narrow-Line Regions of Seyfert 1 and Seyfert 2 Galaxies
A Complete Atlas of Recalibrated Hubble Space Telescope Faint Object Spectrograph Spectra of Active Galactic Nuclei and Quasars. I. Pre-COSTAR Spectra
HST Observations of NGC 4395, the Least Luminous Seyfert 1 Nucleus: Evidence against the Starburst Hypothesis for Broad-lined Active Galactic Nuclei
Observations of O I and Ca II Emission Lines in Quasars: Implications for the Site of Fe II Line Emission
On the Effects of Dissipative Turbulence on the Narrow Emission-Line Ratios in Seyfert Galaxies
On the nature of the near-UV extended light in Seyfert galaxies
Physical Conditions in the Emission-Line Gas in the Extremely Low Luminosity Seyfert Nucleus of NGC 4395
The Redshifted Excess in Quasar C IV Broad Emission Lines
Instrument
FOS/BL, FOS/RD, WFPC/PC
Temporal Coverage
1992-07-15T03:08:59Z/1992-07-19T08:49:11Z
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, Filippenko comma Alex V., 1993, 'ULTRAVIOLET SPECTROSCOPY AND HIGH-RESOLUTION IMAGING OF NGC 4395, THE LEAST LUMINOUS AND NEAREST KNOWN SEYFERT 1 NUCLEUS', 1.0, European Space Agency, https://doi.org/10.5270/esa-2bxn8jc