SED for the unabsorbed optical through γ-ray emission from J1741. The cold BB, hot BB, and broken PL model components are shown by red-orange, orange, and blue lines, respectively, the corresponding shaded areas show the 1σ uncertainties of the model components in the ranges where the pulsar was observed. The purple lines and shaded area show the γ-ray model and its 1σ uncertainties, whereas the light purple shaded area shows the continuation of the γ-ray model toward lower energies. The blue solid line shows the best-fit model to the optical-UV and X-ray data.