Fig. G.1.
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SED fit of observed fluxes in UVIT, GALEX, UVOT, UVBRI, Gaia DR3, APASS, DENIS, 2MASS, and WISE filters (30 photometric fluxes in total from UV to IR) for the PAGB star. The coloured solids are the observed fluxes, the black solids are the best-fitting model fluxes, and the grey solid is the best-fitting TLUSTY model grid spectra.
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