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This galaxy is supposed to be very old, suspected to include dark matter, and likely formed the bulk of its stars before the reionisation of the Universe.\n  New abundances have been obtained from observations of Pisces II 10694 at the Kueyen ESO VLT telescope, using the high-efficiency spectrograph: X-Shooter.\n  We found that Pisces II 10694 is a CEMP-no star with [Fe/H]=-2.60 dex. 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