2003
DOI: 10.1016/s0039-6028(03)00464-3
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Geometrical characterization of pyrimidine base molecules adsorbed on Cu() surfaces: XPS and NEXAFS studies

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Cited by 62 publications
(62 citation statements)
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“…For the initial room temperature deposited layer Fig. 3 agrees well with the previously-reported O 1s and N 1s SXPS [8] although there are differences in absolute binding energies of ~0.5 eV. This is probably attributable to differences in calibration methods; in our case the absolute energy calibrations was based on the Cu 3s peaks taken to have a photoelectron binding energy of 122.45 eV [16,17].…”
Section: Spectral Characterisation: Sxps and Nexafssupporting
confidence: 85%
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“…For the initial room temperature deposited layer Fig. 3 agrees well with the previously-reported O 1s and N 1s SXPS [8] although there are differences in absolute binding energies of ~0.5 eV. This is probably attributable to differences in calibration methods; in our case the absolute energy calibrations was based on the Cu 3s peaks taken to have a photoelectron binding energy of 122.45 eV [16,17].…”
Section: Spectral Characterisation: Sxps and Nexafssupporting
confidence: 85%
“…4 shows the O K-edge NEXAFS spectra recorded at grazing incidence, and at normal incidence in each of the two principle azimuths, from thymine adsorbed on Cu(110) at room temperature, and in a single azimuthal plane from a deposition at ~530 K. The photon energy calibration used in preparing these spectra is based on a very weak O Kedge feature in the incident flux attributable to O contamination in the optics. This feature was assigned an energy of 531 eV; while this calibration method is far from exact, the resulting room temperature preparation data are in excellent agreement with those of Furukawa et al [8]. Notice that the incident beam is horizontal (with a horizontal plane of polarisation), so as the angle of incidence is varied by rotating the sample about a vertical axis, the azimuth of the incidence plane is also the azimuth of the polarisation vector of the incident radiation.…”
Section: Spectral Characterisation: Sxps and Nexafssupporting
confidence: 76%
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“…The C 1s spectra and also N 1s, O 1s, and P 2p do not show any changes for DNA kept in ultrahigh vacuum conditions after 6 h. Previous studies reported 1s core electron binding energies for selected elements of different species, i.e., C 1s spectra were recorded for condensed phase of all nucleobases, 13,15 N 1s for thymine 15,16 and guanine, 15 and O 1s for cytosine 16 and thymine. 15,16 In the present work, high resolution C 1s spectra of DNA nucleobases are shown in Fig. 2 and exhibit a complicated structure due to contributions from different molecular species containing carbon atoms.…”
Section: A Xps Characterization Of Nucleobasesmentioning
confidence: 68%