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Measurements of the Ultraviolet Spectral Characteristics of Low-mass Exoplanetary Systems ("MUSCLES")

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Mendeley Data2024-06-25 更新2024-06-27 收录
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http://archive.stsci.edu/doi/resolve/resolve.html?doi=10.17909/T9DG6F
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MUSCLES is a spectral survey of 11 low-mass, planet-hosting stars, 7 M and 4 K dwarfs. The spectra cover wavelengths from 5 Angstroms to 5.5 microns, with emphasis on high-energy radiation. Data sources for the various regions of the spectra include 1.) X-rays: Chandra/XMM-Newton and APEC models (Smith et al. 2001) 2.) EUV: Empirical scaling relation based on Lya flux (Linsky et al. 2014) 3.) Lyman alpha: Reconstructed from model fit to line wings (Youngblood et al., 2016) 4.) FUV - blue visible: HST COS and STIS 5.) Visible - IR: Synthetic photospheric spectra from PHOENIX atmosphere models (Husser et al. 2013).
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2023-06-28
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