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18 May 2022: conductivities:one lower and one higher than the 200 lS/cm of our NP batches. ... It results in a cloud with average NPcenter-to-center separations of 200 nm and, thus, saturates the NPdensity in the cloud.

23 Sep 2022: z (nm). 100μm 500nm. 200. 100. 0. 0.5 1 1.5 2. ... 1000020000. Position (μm)1000 200 300 400. 0. 100. 200H. eigh. t (nm. ).

11 May 2022: Scale bars are 300 μm, 300 μm, 150 μm, 100 μm, 100 μm, 200 μm, 300 μm, 5 mm, and 100 μm in ... Scale bars are 200 μm, 200 μm, 80 μm, and 40 μm in (a,b,e,f ) respectively.

11 Feb 2022: In suchsystems strong light-matter coupling gives rise to polaritonsplittings on the order of 200 to 300 meV6. ... followed by a slower expansion over the fol-lowing 200 fs, labelled R2.

2 Dec 2022: These latter peaks have a distinctly narrower FWHM (from 200 cm1 to <20–50 cm1, SI Appendix, Tables S2 and S3) characteristic of discrete water clusters (2, 35). ... Raman measurements from 200 to 700 cm1 can access librational motions, key to hydrogen

27 Jun 2022: measurements using NPoM tracking software (35), with power-series laser irradiation from 2 to 200 W on many different NPoMs across each sample (Fig. ... 3, B  and  F) are extracted from the distribution of lifetimes (Tp spans 200 ms to 180 s) by

19 Jan 2022: z (n. m). E/E 0. 200 nm. ΔT. 0. 0.5. –10.

4 Feb 2022: laser isscanned across the photoresist, resulting in the writing ofdevice features below 200 nm in lateral size. ... The sample was excitedusing a 488 nm wavelength laser (Cobolt 06-MLD, 200 mW diodelaser, Cobolt), which was directed to the back aperture

12 Jul 2022: Results are normalized to values at theweakest intensity considered and are obtained with g0 = 1 meV, ωres=1.72 eV, κ = 200 meV, ωvib = 196.5 meV, γvib = 0.07 meV, ... signal30 could reconcile themeasurements and the predictions from molecular

28 Jun 2022: STEM mode (200 kV acceleration voltage) using a FIB-TEM HeliosNanolab 450S in SAE Technologies Development (Dongguan) Co.,Ltd., Guangdong Province, China. ... g) (200)Bragg reflex in q space. (h) Photoluminescence spectra of CsPbBrxI3‑x NC thin films