A Search for H I Lya Counterparts to Ultrafast X-Ray Outflows
Bias in C IV-based quasar black hole mass scaling relationships from reverberation mapped samples
Calibrating C-IV-based Black Hole Mass Estimators
Characterizing Transition Temperature Gas in the Galactic Corona
C IV Line-width Anomalies: The Perils of Low Signal-to-noise Spectra
Extending the Calibration of C IV-based Single-epoch Black Hole Mass Estimators for Active Galactic Nuclei
Intervening broad-line region clouds effects on the optical/ultraviolet spectrum
Linking the power sources of emission-line galaxy nuclei from the highest to the lowest redshifts
The continuum and narrow-line region of the narrow-line Seyfert 1 galaxy Mrk 766
The X-ray/UV absorber in NGC 4593
Ultraviolet and Optical Properties of Narrow-Line Seyfert 1 Galaxies
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-04-11T16:02:24Z/2002-06-24T03:55:47Z
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, Kaiser comma Mary Elizabeth, 2006, 'UV ABSORPTION IN AN XRAY SELECTED SAMPLE OF SEYFERT 1 GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-1puwvwf