1989
DOI: 10.1103/physreva.40.652
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K-edge near-edge x-ray-absorption fine structure of oxygen- and carbon-containing molecules in the gas phase

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Cited by 108 publications
(92 citation statements)
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“…Furthermore, the functional and other subgroups in such large compositions are regarded as independent units. But each of these units has its ionization point at another energy, as known from the literature (Francis and Hitchcock 1992;Hitchcock 1987, 1988;Sham et al 1989;Stöhr 1992;Kikuma and Tonner 1996). Thus, due to a mix of chemistries leading to chemical shifts of the core level, the arctangent for large and complex molecules like environmental samples would be very broad, and thereby dominate the fit of the spectra and submerging the Gaussian curves, see Fig.…”
Section: Analysis Of the Spectramentioning
confidence: 99%
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“…Furthermore, the functional and other subgroups in such large compositions are regarded as independent units. But each of these units has its ionization point at another energy, as known from the literature (Francis and Hitchcock 1992;Hitchcock 1987, 1988;Sham et al 1989;Stöhr 1992;Kikuma and Tonner 1996). Thus, due to a mix of chemistries leading to chemical shifts of the core level, the arctangent for large and complex molecules like environmental samples would be very broad, and thereby dominate the fit of the spectra and submerging the Gaussian curves, see Fig.…”
Section: Analysis Of the Spectramentioning
confidence: 99%
“…However, as seen from NEXAFS spectra of small, well-understood molecules Hitchcock 1987, 1988;Sham et al 1989;Cooney and Urquhart 2004;Kolczewski et al 2006;Bâldea et al 2007;Solomon et al 2009), shifts of peak positions and absorption edges occur, depending on, e.g., the chemical environment, the substrate, or the state of aggregation. Furthermore, the functional and other subgroups in such large compositions are regarded as independent units.…”
Section: Analysis Of the Spectramentioning
confidence: 99%
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“…Ionization energies for OCS are 540.3 eV for O 1s [18], 295.5 eV for C 1s [19], and 170.3 and 171.6 eV for S 2p 3=2 and 2p 1=2 , respectively [19]. About 7.2 eV below the O 1s threshold lies the O 1s !…”
Section: P H Y S I C a L R E V I E W L E T T E R Smentioning
confidence: 99%
“…For example, shifts in peak position were used to discern between oxidized black carbon and organic matter adsorbed to black carbon surfaces Liang et al, 2006). Energy calibration is, for example, done using CO 2 for carbon [with characteristic π*, 3 s, and 3 p peaks at 290.7, 292.74, and 294.96 eV, respectively (Sham et al, 1989;Ma et al, 1991)] and oxygen [with characteristic π* and 3 s peaks at 535.0 and 539.3 eV, respectively (Sham et al, 1989), and 535.4 and 539.0 eV ], using N 2 for nitrogen [with a characteristic 1 s → π*(v = 1) peak (second large peak) at 401.10 eV (Sodhi and Brion 1984)], using variscite [2149 eV (Beauchemin et al, 2003)] for phosphorus, and elemental sulfur [2872 eV (Hutchison et al, 2001;Solomon et al, 2003)] or calcium sulfate (2482.5 eV) for sulfur NEXAFS. Careful measurement of standard substances, explicit mentioning of the energy position to which a standard was calibrated is essential to working with and reporting NEXAFS results.…”
Section: Quantification Of Bonds and Compoundsmentioning
confidence: 99%