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Figure 5
APU22 characteristics for the different harmonics in the energy range between 5.7 and 28 keV at the EMA and the MANACÁ beamlines at Sirius: (a) peak emission energy Eu as a function of the phase pu; (b) variation correlation between Eu and pu as a function of Eu; (c) energy tuning tolerance ratio as a function of pu; and (d) phase error tolerance [\Gamma_{p_{\rm{u}}}] as a function of pu.

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