AGN Narrow-Line Kinematics: Determining Inclinations via Outflows
Chandra Observations of Candidate ``True Seyfert 2 Nuclei
Demystifying the coronal-line region of active galactic nuclei: spatially resolved spectroscopy with the Hubble Space Telescope
Determining Inclinations of Active Galactic Nuclei via their Narrow-line Region Kinematics. I. Observational Results
Gas inflows towards the nucleus of NGC 1358
Gemini Near Infrared Field Spectrograph Observations of the Seyfert 2 Galaxy Mrk 573: In Situ Acceleration of Ionized and Molecular Gas off Fueling Flows
Modeling the Outflow in the Narrow-line Region of Markarian 573: Biconical Illumination of a Gaseous Disk
On a Method to Resolve the Nuclear Activity in Galaxies as Applied to the Seyfert 2 Galaxy NGC 1358
Physical Conditions in the Inner Narrow-Line Region of the Seyfert 2 Galaxy Markarian 573
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. I. Spatially Resolved Mass Outflow Rates for the Seyfert 2 Galaxy Markarian 573
Spatially Resolved Narrow-Line Region Kinematics in Active Galactic Nuclei
The HST view of the innermost narrow line region
The Nuclear Outflows and Feedback in the Seyfert 2 Galaxy Markarian 573
Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
Upper Limits on the Mass of Supermassive Black Holes from Archival Data of the Space Telescope Imaging Spectrograph
Upper limits on the mass of supermassive black holes from HST/STIS archival data.
Instrument
STIS, STIS/CCD
Temporal Coverage
2001-08-11T04:58:48Z/2002-01-25T19:15:35Z
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, Pogge comma Richard W., 2002, 'STIS Spectrophotometry of Nearby Seyfert 2 Nuclei: Can we eliminate the Seyfert 2 class?', 1.0, European Space Agency, https://doi.org/10.5270/esa-0v3yt67