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Fig. 7 (a) Time-resolved infrared (TRIR) spectra of
wt
GFP. Spectra were recorded at 2 ps
(
yellow
), 4 ps (
turquoise
), 10 ps (
brown
), 30 ps (
green
), 100 ps (
blue
), and 200 ps (
red
) after
excitation. Spectra were recorded under magic angle conditions to avoid the influence of polariza-
tion. The main transitions are labeled with their energy. (b, c) Polarization-resolved TRIR for
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