Modeled XUV and FUV spectrum based on the paper by Namekata, Toriumi, Airapetian et al. (2023, submitted to ApJ). These are reconstructed by using the solar scaling relations and the observed stellar magnetic field. The spectra cover the wavelength range of 0.5-180 nm.
-EK Dra (Age of 0.1 Gyr)
-Pi01 UMa (Age of 0.5 Gyr)
-Kappa01 Ceti (Age of 0.6 Gyr)
-Sun (in activity minimum, Age of 4.6 Gyr)
-Sun (in activity maximum, Age of 4.6 Gyr)
-1st: wavelength [nm]; 0.5-180 nm
-2nd: extrapolated XUV/FUV spectra [erg/s/nm/cm^2 at 1 AU]
-3rd: 2nd-yerr
-4th: 2nd+yerr
Last updates...Jan 30th, 2023
Contact: Kosuke Namekata ( namekata_[at mark]_kusastro.kyoto-u.ac.jp )