Hubble Space Telescope STIS Ultraviolet Spectral Evidence of Outflow in Extreme Narrow-Line Seyfert 1 Galaxies. I. Data and Analysis
Hubble Space Telescope STIS Ultraviolet Spectral Evidence of Outflow in Extreme Narrow-Line Seyfert 1 Galaxies. II. Modeling and Interpretation
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
Long XMM observation of the narrow-line Seyfert 1 galaxy IRAS 13224-3809: rapid variability, high spin and a soft lag
Relativistic disc reflection in the extreme NLS1 IRAS13224-3809
Super-Eddington QSO RX J0439.6-5311 - II. Multiwavelength constraints on the global structure of the accretion flow
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-02-16T06:19:35Z/1999-06-06T04:51:36Z
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, Leighly comma Karen Marie, 2007, 'A Search for Broad Absorption Lines in Narrow-Line Seyfert 1 Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-ciu69my