A Census of Near-UV M-dwarf Flares Using Archival GALEX Data and the gPHOTON2 Pipeline
A Chandra/LETGS Survey of Main-sequence Stars
Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Effective Induction Heating around Strongly Magnetized Stars
Far-ultraviolet Flares on Accreting Protostars: Weak and Classical T Tauri Stellar Pair Analysis
Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
From Radio to X-Ray: Flares on the dMe Flare Star EV Lacertae
Modeling Balmer line signatures of stellar CMEs
Multiwavelength Observations of Flares on AD Leonis
Opacity in the upper atmospheres of active stars. II. AD Leonis
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-03-10T03:20:20Z/2000-03-13T09:18:38Z
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, Hawley comma Suzanne L., 2006, 'Coordinated Observations of Stellar Flares on AD Leo', 1.0, European Space Agency, https://doi.org/10.5270/esa-xvxo7iq