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. 2017 Jun 30;8:1227. doi: 10.3389/fmicb.2017.01227

Table 1.

Sample list and alpha diversity.

Sample Name Group ID Type Shock Weathering Nseqs Sobs Coverage Chao∗♢ Inv. Simpson∗♢ Shannon
Watson 021 MA L7 S4 W4 34871 2051 (N/A) 0.9704 (N/A) 3961 (N/A) 22.77 (N/A) 4.734 (N/A)
Watson 022 MB L6 S4 W2 49758 2181 (19) 0.9626 (0.0006) 4935 (177) 23.7 (0.19) 4.592 (0.007)
Watson 019 MC L6 S3 W1 62811 2702 (23) 0.9631 (0.0007) 5233 (177) 29.36 (0.34) 5.390 (0.009)
Watson 020 MD L5 S2 W1 55066 8955 (46) 0.8044 (0.0015) 33057 (837) 57.28 (0.77) 6.747 (0.010)
Soil (Watson 021) SA Soil
Soil (Watson 022) SB Soil 38159 3144 (12) 0.9441 (0.0004) 7699 (156) 24.75 (0.10) 4.915 (0.004)
Soil (Watson 019) SC Soil 57753 12845 (54) 0.6973 (0.0017) 68819 (1679) 101.91 (1.66) 7.616 (0.010)
Soil (Watson 020) SD Soil 60281 15272 (57) 0.6316 (0.0018) 88505 (2075) 342.71 (5.45) 8.190 (0.009)

Student’s t-test was conducted between the meteorite and the soil substrates on Inv. Simpson with a p > 0.05 for both. Standard deviations are given in brackets.

Samples were subsampled to the library size of MA, which had the lowest number of sequences: 34871. Names of all meteorites are still waiting official classification by the Meteoritical Bulletin.