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The spectral dependencies of the photogeneration efficiencies of vapor-deposited amorphous layers of PECI. The efficiencies were computed on an incident photon basis.

The spectral dependencies of the photogeneration efficiency of a dual-layer aggregate photoreceptor on an incident and absorbed photon basis.

The spectral dependencies of the xerographic gain of a series of chalcogenide glass photoreceptors.

The spectral energy distributions of various galaxy components at the IRAC wavelengths. The IRAC bandpasses are shown at the bottom of the figure. Warm dust emitting in the PAH lines, and active nuclei, both appear red in the IRAC bandpasses, while stellar light appears blue. The presence of CO absorption in the 4.5 pm bandpass also results in cool, late-type stars having a bluer color — than earlier-type stars like Vega.

The spectral evidence of the formation of hydroperoxide Si-O-O-H groups in reaction DOSG with water molecules, appearance of a structureless wing of a UV band whose form is close to that observed in absorption spectrum of the HOOH molecule.

The spectral features in this region originate from the formic acid dimer 2.

The spectral features in this region originate from the formic acid dimer HCOOHh-

The spectral function of He-Ar pairs at 295 K, computed from first principles, compared with the experiment dots, .

The spectral functions derived from the measurements,

The spectral intensities of the methylene resonance , the

The spectral intensities of the methylene resonsance of DPPC GMi 1.0 M

The spectral manifestation of intercollision anticorrelation. Curve I is the spectral density of the force F acting in liquid , curve II the same but in the approximation of independent collisions.

The spectral manifestation of the Raman effect, The Raman spectrum. The relative intensities of the incident, Rayleigh, and Raman hnes are quite different in real

The spectral moment y as function of the product of densities, for various rare-gas mixtures at room temperature only one density was varied for each system

The spectral position of the laser emission and the threshold curves unetched resonator with OD 75 pm and the wall thickness of 5 pm with a threshold of 25 nJ mm2. Reprinted from Ref. 20 with permission. 2008 International Society for Optical Engineering

The spectral power distribution curves of standard CIE illuminants. Figure courtesy of GretagMacbeth. This black and white facsimile of the figure is intended only as a placeholder for full-color version of figure go to httptfwww.currentprotocols.com colorfigures

The spectral power distribution of a fluorescent lamp containing two rare earth phosphors, those of Figures 1 , and green-emitting zinc silicate

The spectral radiance of a blackbody at various temperatures from top to bottom 2000, 1500, and 1000 K,

The spectral range covered by different tunable solid state lasers based on transition metal ions.

The spectral range covered by the fundamental radiation of a Ti-sapphrre laser and the various harmonic generation processes

The spectral range of laser emission for several semiconductor materials.

The spectral reflectance curve of a red object plots reflectance at each wavelength. Figure courtesy of GretagMacbeth. This black and white facsimile of the figure is intended only as a placeholder for full-color version of figure go to http

The spectral reflectance of CBCF and etched beryllium over the wavelength range 2 to 55 pm .

The spectral reflectivity of the sensing film measured over the range 400 1,000 nm before

The spectral region between 4.3 and 5.4 ppm is significantly more



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