Current Population Statistics Do Not Favor Photoevaporation over Core-powered Mass Loss as the Dominant Cause of the Exoplanet Radius Gap
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Estimating the Ultraviolet Emission of M Dwarfs with Exoplanets from Ca II and Ha
HAZMAT. IV. Flares and Superflares on Young M Stars in the Far Ultraviolet
HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear
HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars
HAZMAT VI: The Evolution of Extreme Ultraviolet Radiation Emitted from Early M Stars
Nonthermal Motions and Atmospheric Heating of Cool Stars
Optically quiet, but FUV loud: results from comparing the far-ultraviolet predictions of flare models with TESS and HST
The M-dwarf Ultraviolet Spectroscopic Sample. I. Determining Stellar Parameters for Field Stars
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2017-07-19T18:37:28Z/2019-03-30T09:57:08Z
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, Shkolnik comma Evgenya L., 2019, 'HAZMAT: Habitable Zones and M dwarf Activity across Time', 1.0, European Space Agency, https://doi.org/10.5270/esa-79jnctp
