Fig. D.1.
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Disentangled simulated spectra for a 45 000 K stripped star with different contributions. Black: the models. Blue: the disentangled spectra given a 1% contributed flux. Orange: a 3% contributed flux. Green: for a 5% contributed flux. The model in the left panels is for a B star of 19 000 K and v sin i = 330 km s−1. The model in the middle and right panels is for a stripped star of 45 000 K and v sin i = 30 km s−1.
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