Fig. 5
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Spectral energy distributions of our three target stars. Observed photometry is shown by blue boxes and the spectrum of the best-fitting model by a red dashed line. Photometry is from GALEX (FUV and NUV), Gaia DR3 (Gbp), Pan-STARRS (PSg, PSr, PSi, PSz, Psy), and 2MASS (J, H, KS). For comparison the resulting photometric values from the models are also shown as red boxes.
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