000167831 001__ 167831
000167831 005__ 20250730152357.0
000167831 0247_ $$2doi$$a10.1016/j.jlumin.2012.08.052
000167831 0247_ $$2ISSN$$a1872-7883
000167831 0247_ $$2ISSN$$a0022-2313
000167831 0247_ $$2WOS$$aWOS:000313393300028
000167831 0247_ $$2openalex$$aopenalex:W2129351338
000167831 037__ $$aDESY-2014-02157
000167831 082__ $$a530
000167831 1001_ $$0P:(DE-H253)PIP1007370$$aZych, Aleksander$$b0$$eCorresponding author
000167831 245__ $$aAnalysis of the shift of zero-phonon lines for f–d luminescence of lanthanides in relation to the Dorenbos model
000167831 260__ $$aNew York, NY [u.a.]$$bElsevier$$c2013
000167831 3367_ $$2DRIVER$$aarticle
000167831 3367_ $$2DataCite$$aOutput Types/Journal article
000167831 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1527520214_11072
000167831 3367_ $$2BibTeX$$aARTICLE
000167831 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000167831 3367_ $$00$$2EndNote$$aJournal Article
000167831 500__ $$a(c) Elsevier B.V.; Post referee fulltext in progress; Embargo 12 months from publication
000167831 520__ $$aThe Dorenbos relation is an empirical model that relates the position of the lowest fd level of any lanthanide ion with that of Ce3+ in the same host lattice. The relation is widely used to estimate the energy of fd levels of trivalent lanthanide ions in a given host lattice based on the peak position of the lowest fd level of at least one of the lanthanide ions in that host. The energy of fd levels is determined from peak maxima in excitation and emission spectra. In this work we use the position of zero-phonon lines (ZPLs) as input to investigate the accuracy of the Dorenbos relation. To this end, the ZPL positions of the fd bands for trivalent lanthanide ions in four different host lattices (CaF2, Y3Al5O12, LiYF4, and YPO4) were obtained and used as input in the Dorenbos relation. The results are compared to those obtained through the standard procedure using band maxima. The data indicate that the ZPL approach gives more accurate estimates for the position of the lowest fd level with standard deviations that are 2–3 times smaller than those obtained for band maxima. The results confirm the concept of the Dorenbos model (constant energy difference between the fd levels of lanthanides) and show that the accuracy is even better than previously reported. The main cause for the larger deviation from positions of band maxima is related to a larger inaccuracy in determining band maxima compared to ZPLs.
000167831 536__ $$0G:(DE-H253)POF2-I-20130405$$aDORIS Beamline I (POF2-54G13)$$cPOF2-54G13$$fPOF II$$x0
000167831 588__ $$aDataset connected to CrossRef, bib-pubdb1.desy.de
000167831 693__ $$0EXP:(DE-H253)D-I-20150101$$1EXP:(DE-H253)DORISIII-20150101$$6EXP:(DE-H253)D-I-20150101$$aDORIS III$$fDORIS Beamline I$$x0
000167831 7001_ $$0P:(DE-HGF)0$$aOgieglo, Joanna$$b1
000167831 7001_ $$0P:(DE-HGF)0$$aRonda, Cees$$b2
000167831 7001_ $$0P:(DE-HGF)0$$aMello Donegá, Celso de$$b3
000167831 7001_ $$0P:(DE-H253)PIP1008235$$aMeijerink, Andries$$b4
000167831 773__ $$0PERI:(DE-600)1491401-3$$a10.1016/j.jlumin.2012.08.052$$gVol. 134, p. 174 - 179$$p174 - 179$$tJournal of luminescence$$v134$$x0022-2313$$y2013
000167831 8564_ $$uhttps://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.pdf$$yRestricted
000167831 8564_ $$uhttps://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-1440$$xicon-1440$$yRestricted
000167831 8564_ $$uhttps://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-180$$xicon-180$$yRestricted
000167831 8564_ $$uhttps://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-640$$xicon-640$$yRestricted
000167831 909CO $$ooai:bib-pubdb1.desy.de:167831$$pVDB
000167831 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1007370$$aExternes Institut$$b0$$kExtern
000167831 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1008235$$aExternes Institut$$b4$$kExtern
000167831 9131_ $$0G:(DE-HGF)POF2-54G13$$1G:(DE-HGF)POF2-540$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$9G:(DE-H253)POF2-I-20130405$$aDE-H253$$bStruktur der Materie$$lForschung mit Photonen, Neutronen, Ionen$$vDORIS III$$x0
000167831 9141_ $$y2013
000167831 915__ $$0StatID:(DE-HGF)0010$$2StatID$$aJCR/ISI refereed
000167831 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR
000167831 915__ $$0StatID:(DE-HGF)0110$$2StatID$$aWoS$$bScience Citation Index
000167831 915__ $$0StatID:(DE-HGF)0111$$2StatID$$aWoS$$bScience Citation Index Expanded
000167831 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection
000167831 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bThomson Reuters Master Journal List
000167831 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000167831 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000167831 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz
000167831 915__ $$0StatID:(DE-HGF)1040$$2StatID$$aDBCoverage$$bZoological Record
000167831 9201_ $$0I:(DE-H253)HAS-User-20120731$$kDOOR$$lDOOR-User$$x0
000167831 980__ $$ajournal
000167831 980__ $$aVDB
000167831 980__ $$aI:(DE-H253)HAS-User-20120731
000167831 980__ $$aUNRESTRICTED