A Far Ultraviolet Spectroscopic Explorer Survey of Late-Type Dwarf Stars
A study of velocity fields in the transition region of e Eri (K2 V)
Chemical Consequences of the C/O Ratio on Hot Jupiters: Examples from WASP-12b, CoRoT-2b, XO-1b, and HD 189733b
CoolCAT
Coronal Emission Measures and Abundances for Moderately Active K Dwarfs Observed by Chandra
Correlating Intrinsic Stellar Parameters with Mg II Self-reversal Depths
Detection of magnetic dipole lines of Fexii in the ultraviolet spectrum of the dwarf star e Eri
Disequilibrium Carbon, Oxygen, and Nitrogen Chemistry in the Atmospheres of HD 189733b and HD 209458b
Fe II fluorescence in main-sequence K-dwarfs
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
OI line emission in cool stars: calculations using partial redistribution
Physical structure of the local interstellar medium
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
The corona and upper transition region of epsilon Eridani
The electron pressure in the outer atmosphere of e Eri (K2 V)
The emission line near 1319 A in solar and stellar spectra
The interstellar cloud surrounding the Sun: a new perspective
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
The three-dimensional physical structure of the local interstellar medium
UV and EUV observations of stellar coronal structure and activity
What Is the Total Deuterium Abundance in the Local Galactic Disk?
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-03-17T21:35:35Z/2000-03-18T01:34:13Z
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, Jordan et al., 2001, 'Epsilon Eri: Structure and Non-Thermal Heating', 1.0, European Space Agency, https://doi.org/10.5270/esa-1ggg2wh