Image Details
Caption: Figure 6.
Spectral energy distribution for Ross 19A. Our KAST and SpeX spectra for Ross 19A are plotted as red and black lines, respectively. All photometry is labeled as in the figure legend and includes GALEX NUV, Gaia G Bp, G, G Rp, 2MASS J, H, K S, and WISE W1, W2, W3, and W4 magnitudes. This comprehensive SED is used to determine fundamental parameters of Ross 19A following the methods in Filippazzo et al. (2015).
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