001     167831
005     20250730152357.0
024 7 _ |a 10.1016/j.jlumin.2012.08.052
|2 doi
024 7 _ |a 1872-7883
|2 ISSN
024 7 _ |a 0022-2313
|2 ISSN
024 7 _ |a WOS:000313393300028
|2 WOS
024 7 _ |a openalex:W2129351338
|2 openalex
037 _ _ |a DESY-2014-02157
082 _ _ |a 530
100 1 _ |a Zych, Aleksander
|0 P:(DE-H253)PIP1007370
|b 0
|e Corresponding author
245 _ _ |a Analysis of the shift of zero-phonon lines for f–d luminescence of lanthanides in relation to the Dorenbos model
260 _ _ |a New York, NY [u.a.]
|c 2013
|b Elsevier
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1527520214_11072
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a (c) Elsevier B.V.; Post referee fulltext in progress; Embargo 12 months from publication
520 _ _ |a The 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.
536 _ _ |0 G:(DE-H253)POF2-I-20130405
|f POF II
|x 0
|c POF2-54G13
|a DORIS Beamline I (POF2-54G13)
588 _ _ |a Dataset connected to CrossRef, bib-pubdb1.desy.de
693 _ _ |a DORIS III
|f DORIS Beamline I
|1 EXP:(DE-H253)DORISIII-20150101
|0 EXP:(DE-H253)D-I-20150101
|6 EXP:(DE-H253)D-I-20150101
|x 0
700 1 _ |a Ogieglo, Joanna
|0 P:(DE-HGF)0
|b 1
700 1 _ |a Ronda, Cees
|0 P:(DE-HGF)0
|b 2
700 1 _ |a Mello Donegá, Celso de
|0 P:(DE-HGF)0
|b 3
700 1 _ |a Meijerink, Andries
|0 P:(DE-H253)PIP1008235
|b 4
773 _ _ |a 10.1016/j.jlumin.2012.08.052
|g Vol. 134, p. 174 - 179
|0 PERI:(DE-600)1491401-3
|p 174 - 179
|t Journal of luminescence
|v 134
|y 2013
|x 0022-2313
856 4 _ |u https://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-1440
|x icon-1440
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-180
|x icon-180
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/167831/files/DESY-2014-02157.jpg?subformat=icon-640
|x icon-640
|y Restricted
909 C O |p VDB
|o oai:bib-pubdb1.desy.de:167831
910 1 _ |a Externes Institut
|0 I:(DE-HGF)0
|k Extern
|b 0
|6 P:(DE-H253)PIP1007370
910 1 _ |a Externes Institut
|0 I:(DE-HGF)0
|k Extern
|b 4
|6 P:(DE-H253)PIP1008235
913 1 _ |b Struktur der Materie
|1 G:(DE-HGF)POF2-540
|0 G:(DE-HGF)POF2-54G13
|2 G:(DE-HGF)POF2-500
|v DORIS III
|9 G:(DE-H253)POF2-I-20130405
|x 0
|a DE-H253
|4 G:(DE-HGF)POF
|3 G:(DE-HGF)POF2
|l Forschung mit Photonen, Neutronen, Ionen
914 1 _ |y 2013
915 _ _ |a JCR/ISI refereed
|0 StatID:(DE-HGF)0010
|2 StatID
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
915 _ _ |a WoS
|0 StatID:(DE-HGF)0110
|2 StatID
|b Science Citation Index
915 _ _ |a WoS
|0 StatID:(DE-HGF)0111
|2 StatID
|b Science Citation Index Expanded
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Thomson Reuters Master Journal List
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0300
|2 StatID
|b Medline
915 _ _ |a Nationallizenz
|0 StatID:(DE-HGF)0420
|2 StatID
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1040
|2 StatID
|b Zoological Record
920 1 _ |0 I:(DE-H253)HAS-User-20120731
|k DOOR
|l DOOR-User
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)HAS-User-20120731
980 _ _ |a UNRESTRICTED


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21