Spectroscopy 1976
DOI: 10.1007/978-94-009-5741-1_6
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Astrochemistry

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Cited by 3 publications
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“…From the quantum yields Φ em and the τ lifetime values, the radiative decay rate ( k r ), the nonradiative decay rate ( k nr ), and the pure radiative lifetime (τ r ) were calculated for a series of complexes through the equations k r = Φ em /τ, k nr = (1 – Φ em )/τ, and τ r ≈ τ/Φ em (see Table ). Thus, the emission quantum yield (Φ em ) is generally formulated as Φ em = k r /( k r + k nr ).…”
Section: Resultsmentioning
confidence: 99%
“…From the quantum yields Φ em and the τ lifetime values, the radiative decay rate ( k r ), the nonradiative decay rate ( k nr ), and the pure radiative lifetime (τ r ) were calculated for a series of complexes through the equations k r = Φ em /τ, k nr = (1 – Φ em )/τ, and τ r ≈ τ/Φ em (see Table ). Thus, the emission quantum yield (Φ em ) is generally formulated as Φ em = k r /( k r + k nr ).…”
Section: Resultsmentioning
confidence: 99%
“…Infrared spectroscopy, however, is not without its drawbacks. It is well-known that glass is quite unsuitable for any type of optics (e.g., lenses, widows, or sample slides) because of its opacity over most of the useful mid-infrared region of the spectrum. In order to analyze a biopsy sample, therefore, the slice of tissue either has to be placed on a mid-infrared transparent substrate such a calcium fluoride (CaF 2 ) or barium fluoride (BaF 2 ) for a transmission measurement or on a highly reflecting substrate for a, so-called, transflection measurement. In the case of a transmission measurement the substrates are expensive (typically greater than $40 per slide) and are far from robust.…”
mentioning
confidence: 99%
“…Astronomical objects produce spectra in both emission and absorption (Thackeray 1961, Straughan andWalker 1976). The simulator does the same, generating an array of 'stars' in an imaginary constellation by various methods.…”
Section: The Stellar Spectra Simulatormentioning
confidence: 99%