A Census of Near-UV M-dwarf Flares Using Archival GALEX Data and the gPHOTON2 Pipeline
Computing Intrinsic LYa Fluxes of F5 V to M5 V Stars
Correlating Intrinsic Stellar Parameters with Mg II Self-reversal Depths
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets around Low-mass Stars: GJ 832, GJ 176, and GJ 436
Semiempirical Modeling of the Atmospheres of the M Dwarf Exoplanet Hosts GJ 832 and GJ 581
Semi-empirical Modeling of the Photosphere, Chromosphere, Transition Region, and Corona of the M-dwarf Host Star GJ 832
The MUSCLES Treasury Survey. II. Intrinsic LYa and Extreme Ultraviolet Spectra of K and M Dwarfs with Exoplanets*
The MUSCLES Treasury Survey. III. X-Ray to Infrared Spectra of 11 M and K Stars Hosting Planets
The MUSCLES Treasury Survey. I. Motivation and Overview
The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs
The Ultraviolet Radiation Environment around M dwarf Exoplanet Host Stars
The ultraviolet radiation environment in the habitable zones around low-mass exoplanet host stars
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2011-07-09T23:44:06Z/2011-09-04T04:11:50Z
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, Green et al., 2012, 'COS-GTO: Activity of Solar Mass Stars from Cradle to Grave Part 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-n1r3ld0
