An HST COS SNAPshot Spectrum of the K Supergiant l Vel (K4Ib-II)
Computing Intrinsic LYa Fluxes of F5 V to M5 V Stars
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Far-ultraviolet Continuum Emission: Applying This Diagnostic to the Chromospheres of Solar-mass Stars
Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
In the Trenches of the Solar-Stellar Connection. VI. Total EclipSS
Nonthermal Motions and Atmospheric Heating of Cool Stars
The Amazing COS FUV (1320 - 1460 A) Spectrum of l Vel (K4Ib-II)1
The Curious Case of the Alpha Persei Corona: A Dwarf in Supergiants Clothing?
The Flare-ona of EK Draconis
Ultraviolet Spectroscopy of Rapidly Rotating Solar-Mass Stars: Emission-line Redshifts as a Test of the Solar-Stellar Connection
Warm Coronal Rain on Young Solar Analog EK Draconis?
Instrument
COS, COS/FUV
Temporal Coverage
2009-10-12T00:47:25Z/2010-07-18T10:51:31Z
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.
