  We provide ingredients and recipes for computing neutrino signals of
TeV-scale Dark Matter annihilations in the Sun. For each annihilation channel
and DM mass we present the energy spectra of neutrinos at production,
including: state-of-the-art energy losses of primary particles in solar matter,
secondary neutrinos, electroweak radiation. We then present the spectra after
propagation to the Earth, including (vacuum and matter) flavor oscillations and
interactions in solar matter. We also provide a numerical computation of the
capture rate of DM particles in the Sun. These results are available in
numerical form.
