Fig. B.1.
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Same as Fig. 5, now including models. The solid lines and open triangles are models for star formation bursts. The dotted lines and open squares are models for continuous star formation. The red models include VMS (present study), the blue models are BPASS, and the cyan models are from Schaerer & Vacca (1998). The pink models are the VMS models that include nebular continuum emission.
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