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Fig. 26.
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BP and RP spectra of the 20 randomly chosen (amongst 254) carbon stars (this work) with Teff GSP − Phot > 6000 K. The ordinate axis provides the flux normalised to the total flux, and shifted by k × 0.003 (where k is an integer that varies from 0 to 9 from the bottom to the top spectrum).
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