The spectral-energy distribution for BD+14°3061, corrected for interstellar extinction. The fluxes are taken from GALEX (fuv and nuv), APASS (ugriz), my V magnitude, 2MASS (JHK_s), and WISE (3.4, 4.6, 12, and 22 μm). Also plotted is a blackbody with a temperature of 6000 K, normalized to the flux of BD+14°3061 at the V band. There is no evidence for significant circumstellar dust.