Sentence examples for thin spectra from inspiring English sources

The minimum variance property associated to thin spectra could be useful for information processing, provide optimal modularity for V1 hypercolumns, and be a first step toward a mathematical definition of hypercolumns.

Although this is far from being an infinitely thin spectrum, it is not absurd to look at the extreme situation where we impose the spectral thinness to be zero.

Thin film spectra were collected with a signal-to-noise ratio of 30 using a 0.25 s acquisition time.

This spectrum also resembles the peak observed in its bulk sample, but some other modes of vibrations are also observed in thin films spectra which are not well resolved in bulk samples.

When used at non-normal incident situation, optical thin film spectrum curve will exhibit strong polarization deviation.

It can be seen that the emission intensity of Ga2O3 thin film luminescence spectra (at approximately 2.1 eV) was lower than the peak intensity of optical bandgap of the reflectance spectra (at 3.4 eV).

Thin film XRD spectra of the ZnO NW arrays were taken on a PANalytical X'Pert PRO diffractometer (Almelo, The Netherlands) operating in the θ to 2θ Bragg configuration using CuKα (λ = 1.5405 Ǻ) radiation.

The new observations confirm the X-ray luminosity detected by ROSAT (LX ∼ 1032 erg s−1) and the hardness of their X-ray spectra (thin thermal with kT ∼ 8 10 keV or power law with photon index of ∼1.7) which are both unusual for normal early type stars.

Solutions of SOD1 at a concentration of 0.3 0.5 mg/ml were deposited on the surface of a germanium prism and dried to form a thin film, and spectra were acquired.

Thin film optical spectra were measured with a Shimadzu UV-3100 spequippedtometer equipped with an ISR-2600Plus integrating sphere.

We begin by re-examining the effect of variable PCBM content in PBTTT blend thin film absorption spectra which will be useful later for selection of resonance Raman excitation schemes (vide infra).