Fig. 3. Left panel: deviation of (A) 1Hα, (B) 13Cα, (C) amide carbonyl chemical shifts from random coil values and (D) the SSP (secondary structure propensity) scores. In (D) positive scores indicate helical propensity while negative values suggest formation of non-helical type PreSMos. Right panel: 1H–15N heteronuclear NOEs (E), backbone 15N relaxation times, T1 (F), T2 (G), and temperature coefficients of the backbone amide hydrogens (H). The horizontal lines in (F) and (G) indicate an average value.
