2012
DOI: 10.1016/j.ijms.2011.09.001
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Zinc isotope fractionation analyses by thermal ionization mass spectrometry and a double spiking technique

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Cited by 11 publications
(5 citation statements)
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“…Substantial progress was achieved after the introduction of the double spike technique for the correction of mass bias, which further reduced the external precision down to 0.04& (Bermin et al, 2006). Moreover, the same reproducibility of 0.04& was achieved using TIMS and the double spike method to determine Zn stable isotopes in natural samples (Ghidan & Loss, 2012).…”
Section: Determination Of Zn Stable Isotopesmentioning
confidence: 99%
“…Substantial progress was achieved after the introduction of the double spike technique for the correction of mass bias, which further reduced the external precision down to 0.04& (Bermin et al, 2006). Moreover, the same reproducibility of 0.04& was achieved using TIMS and the double spike method to determine Zn stable isotopes in natural samples (Ghidan & Loss, 2012).…”
Section: Determination Of Zn Stable Isotopesmentioning
confidence: 99%
“…The measured isotopic ratios of the Ti standard were normalized to 49 Ti/ 47 Ti = 0.749824, which was calculated by the measured Ti isotope composition of SPEX Ti standard (δ 49/47 Ti = −0.92 ± 0.13‰) relative to SRM 3162a, which has a traceable absolute Ti isotope composition being reported in the literature ( 49 Ti/ 47 Ti = 0.750517 , ). Similarly, isotope ratios of the Zn standard was normalized to 68 Zn/ 66 Zn = 0.66516 (calculated from δ 66/64 Zn = −0.36‰ of the HPS Zn and the reference ratio 68 Zn/ 66 Zn = 0.66540 for IRMM-3702), and the Sn isotope ratios of the Sn standard were normalized to 118 Sn/ 120 Sn = 0.74295 . Then, the normalized ratios were used for the isobaric spike calculation.…”
Section: Methodsmentioning
confidence: 99%
“…These were hypothesised to exhibit up to a maximum of 0.037& deviation in the 26 Mg/ 24 Mg ratio (expressed as d 26 *Mg) as a result of the absence of the short-lived 26 Al isotope which would otherwise have decayed to 26 Mg over the rst 2 Ma aer solar system formation. The same group 189 investigated the 176 Lu-176 Hf decay system using the same instrumentation in order to highlight excess 176 Hf anomalies in chondrite meteorites, equating to a ca. 300 Ma excess in apparent age.…”
Section: Sample Preparationmentioning
confidence: 99%