Fig. 2.
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X-shooter spectrum for the CEMP-no star in our sample, DR20080 (red), at [Fe/H] = −3. For a fair comparison, the X-shooter spectrum of PJ07402 at the same [Fe/H] = −3 is also shown in blue (Starkenburg et al. 2013). However, for the full chemical abundance analysis of PJ07402, here we use a HR UVES spectrum from Jablonka et al. (2015).
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