2001
DOI: 10.1016/s0168-9002(01)00750-1
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Photon-induced fluorescence spectroscopy (PIFS)

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Cited by 36 publications
(34 citation statements)
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“…Being site and state selective [18][19][20][21][22][23][24][25][26], dispersed fluorescence provides extensive information on the emitter and on the initial and final states of the emission process. These advantages are routinely utilized in, e.g., astrophysics to characterize emission lines in small system [37].…”
Section: Resultsmentioning
confidence: 99%
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“…Being site and state selective [18][19][20][21][22][23][24][25][26], dispersed fluorescence provides extensive information on the emitter and on the initial and final states of the emission process. These advantages are routinely utilized in, e.g., astrophysics to characterize emission lines in small system [37].…”
Section: Resultsmentioning
confidence: 99%
“…The nozzle was cooled by a liquid He flow and the temperature was stabilized to ±0.5 K. The degree of condensation, i.e., the ratio of monomers to clusters, was about 50%. The mean cluster size of N 20 = was chosen large enough to enable detectable photon rates with the present advanced single-photon counting technique PIFS [18]. It was controlled following the formula of [27] with the present stagnation pressure of 518 mbar and nozzle temperature of 60 K.…”
Section: Methodsmentioning
confidence: 99%
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“…The UV/visible and VUV photons released in the second and third steps of the cascade (Fig. 1c) were simultaneously detected by the well-established set-up for photon-induced fluorescence-spectroscopy [20] (PIFS). It has already been successfully utilized to investigate autoionization [21,22,23,24,25] and Auger decay [26,27,28,29,30] in molecules.…”
Section: Methodsmentioning
confidence: 99%
“…The experiment was carried out at the undulator beam line UE56/2-PGM2 of BESSY II, Berlin, using photon-induced fluorescence spectroscopy [21,22]. The energy of the exciting synchrotron radiation was varied in steps of 5 meV covering the energy range from resonance R2 to R4 whose energies are 92.425 and 92.560 eV, respectively [17].…”
Section: R2 R4 R1mentioning
confidence: 99%