A Census of Near-UV M-dwarf Flares Using Archival GALEX Data and the gPHOTON2 Pipeline
A Detailed Study of Opacity in the Upper Atmosphere of Proxima Centauri
Atomic Deuterium/Hydrogen in the Galaxy
CoolCAT
H2 Fluorescence in M Dwarf Systems: A Stellar Origin
Observational Estimates for the Mass-Loss Rates of a Centauri and Proxima Centauri Using Hubble Space Telescope Lya Spectra
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
The Direct Detection and Characterization of M-dwarf Planets Using Light Echoes
The full spectral radiative properties of Proxima Centauri
The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants
The habitability of Proxima Centauri b. I. Irradiation, rotation and volatile inventory from formation to the present
The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs
UV and EUV observations of stellar coronal structure and activity
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-05-08T00:50:27Z/2000-05-09T06:03:47Z
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, Linsky comma Jeffrey L., 2006, 'Dynamics and Energetics of Stellar Flares', 1.0, European Space Agency, https://doi.org/10.5270/esa-xihmnkt