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. 2016 May 31;113(24):E3322–E3331. doi: 10.1073/pnas.1603030113

Fig. 6.

Fig. 6.

Plot of the average d/l ratios of the majority of identified chiral meteoritic sugar acids from Table 1. The 5C values are only from Murch 39; this Murchison fragment was more pristine than Murch 52; *, the 6C value is extrapolated based on the d/l trend of 3C → 4C sugar acids.