Dielectronic satellite contributions to Ne VIII and Ne IX K-shell spectra

$K\alpha$ spectra of heliumlike neon and associated lithiumlike, berylliumlike, and boronlike satellite line emission have been observed with a high-resolution crystal spectrometer on the Lawrence Livermore Electron Beam Ion Trap. The $\mathrm{KLL}$ dielectronic recombination satellites were resolved from their He-like parent lines in electron energy space, and their wavelengths and resonance strengths measured. The wavelength measurements achieved a typical accuracy of a few $\mathrm{m}\AA ,$ with two measurements accurate to better than one part in 10 000. By normalizing to the He-like resonance line, w, we measure Li-like satellite resonance strengths that are 10% to 46% lower than predicted by theoretical models. The wavelengths and relative strengths of Be-like $\mathrm{KLL}$ satellites were also measured, and absolute strengths were obtained by normalizing to the collisionally excited Li-like $\mathrm{qr}$ satellite blend.