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Fig. 3
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Matter and CMB (TT, EE, and TE) power spectra computed by SymBoltz (colored lines) compared to CLASS (gray dashes) with relative errors P(k)SymBoltz/P(k)CLASS - 1 and Cl,SymBoltz/Cl,CLASS - 1 for the w0wa CDM model. CLASS uses the precision parameters in Appendix B.
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