Together with the peak at 2θ = 38.1°, the peak at 2θ = 44.3°, (200) reflection lines of cubic Ag, is also observed in the patterns

of the (c) Ag/TiO2-coated wing. Therefore, the amount of deposited Ag for the Ag/TiO2-coated wing seems to be larger than that of the Ag/wing. The crystallinity of the Ag for the Ag/TiO2-coated wing also seems to be higher than that of the Ag/wing. In the XRD patterns of the Ag film, the peaks at 2θ = 38.1° and 44.3° were also clearly seen and the crystallite size of Ag was calculated to be 19.6 nm from the peak (2θ = 38.1°) broadening. On the other hand, the crystallite sizes of Ag nanoparticles deposited on the Ag/wing and Ag/TiO2-coated wing were 12.7 and 22.0 nm, respectively. Therefore, the Ag nanoparticles and Ag film were consisting of small Ag crystallites and the crystallite sizes of Ag nanoparticles deposited on the bare wing and TiO2-coated wing and the Ag films were almost the same. Figure Gefitinib solubility dmso 2 X-ray diffraction patterns of the (a) bare cicada wing, (b) Ag/wing, and (c) Ag/TiO YAP-TEAD Inhibitor 1 2 -coated wing. UV–Vis absorption

spectra of the bare cicada wings, Ag/wings, and Ag/TiO2-coated wings Figure  3 shows the absorption spectra of the (a) bare cicada wing, (b) Ag/wing, and (c) Ag/TiO2-coated wing. In the figure, an absorption peak at 275 nm, due to the nanopillar array structure on the cicada wings is seen for the (a) bare cicada wing [9]. In Figure  3, the (b) Ag/wing and (c) Ag/TiO2-coated wing show the broad LSPR absorption band of the Ag nanoparticles peaking at about 440 nm. The broad absorption bands of the (b) Ag/wing and (c) Ag/TiO2-coated wing suggest that the shape variation and the size distribution

of the Ag nanoparticles are large. In both the spectra, the broad absorption band at a longer wavelength than that of the LSPR peak is probably due to the light scattering of the larger size Ag nanoparticles next of the (b) Ag/wing and (c) Ag/TiO2-coated wing. Figure 3 Optical absorption spectra of the (a) bare cicada wing, (b) Ag/wing, and (c) Ag/TiO 2 -coated wing. SERS spectra of R6G adsorbed on the surface of the bare cicada wings, Ag/wings, Ag/TiO2-coated wings and Ag films SERS spectra of R6G adsorbed on the (a) bare cicada wing, (b) Ag/wing, and (c) Ag/TiO2-coated wing are shown in Figure  4. In this SERS measurement, R6G as standard remarks was adsorbed on the surface at the center of the dorsal forewings with an area of about 54 mm2. The SERS spectrum of R6G adsorbed on the (d) Ag film deposited on a glass slide prepared by sputtering is also shown in Figure  4. In the case of the (d) Ag film, the R6G-adsorbed area was about 50 mm2 which was almost the same as those of the (a) bare cicada wing, (b) Ag/wing, and (c) Ag/TiO2-coated wing. In the figure, R6G adsorbed on the (a) bare cicada wing shows no distinct peaks.