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IR frequencies were calculated using DFT level of theory.
Genotype and allele frequencies were calculated using the χ2 test.
The mean metal particle size of these materials was estimated by HRTEM and turnover frequencies were calculated using these data.
The required vacuum frequencies were calculated using Equations 6 and 7 (see Methods) and the eigenfrequencies recorded in the unbounded fluid, i.e., far from the surface (Table 1).
The average noise levels at high (2.00 4.00 Hz) and low (0.02 0.05 Hz) frequencies were computed, and the RMS amplitudes at these frequencies were calculated using the band-pass-filtered vertical waveforms at IGK.
Haplotypes and haplotype frequencies were calculated using PHASE [34].
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AMOVA analysis based on haplogroup frequencies was calculated using the Arlequin 3.5 software.
Null allele frequencies are calculated using the original genotypes and are based on the excess of homozygous individuals.
The O3-photolysis frequencies were calculated from spectral actinic flux between 290 nm and 340 nm, NO2-photolysis frequencies are calculated using spectral actinic flux between 290 nm and 420 nm.
In most tests, the set of reference frequencies was calculated using all octamers, as described by Tsirigos and Rigoutsos, but in some tests a subset of octamers were used, determined as described above.
Predominance and frequency were calculated using the procedure described by Bodenheimer (1955) in Avendaño and Saíz (1977).
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