Estimating the Ultraviolet Emission of M Dwarfs with Exoplanets from Ca II and Ha
FUMES. III. Ultraviolet and Optical Variability of M-dwarf Chromospheres
FUMES. II. Lya Reconstructions of Young, Active M Dwarfs
Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials
The Far Ultraviolet M-dwarf Evolution Survey. I. The Rotational Evolution of High-energy Emissions
The M-dwarf Ultraviolet Spectroscopic Sample. I. Determining Stellar Parameters for Field Stars
UV Spectral Characterization of Low-mass Stars with AstroSat UVIT for Exoplanet Applications: The Case Study of HIP 23309
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2017-08-22T00:44:33Z/2017-12-27T09:41:28Z
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, Pineda comma John Sebastian, 2018, 'Investigating the FUV Emission of Young M dwarfs with FUMES: the Far Ultraviolet M-dwarf Evolution Survey', 1.0, European Space Agency, https://doi.org/10.5270/esa-j95yg9r