Results 21 to 30 of about 68,403 (337)
Accurate quantification of selenoproteins in human plasma/serum by isotope dilution ICP-MS : focus on selenoprotein P [PDF]
, 2017 Acknowledgements The research leading to these results was funded by the EMRP Joint Research Project “Metrology for metalloproteins” (HLT-05 2012). The EMRP is jointly funded by the EMRP participating countries within EURAMET and the European Union.Peer ...Busto, M. Estela del Castillo, Cuello-Nunez, Susana, Deitrich, Christian L., Fisicaro, Paola, Goenaga-Infante, Heidi, Konopka, Anna, Lehmann, Wolf D., Oster, Caroline, Raab, Andrea +8 morecore +1 more sourceThe Potential of Isotopic Tracers for Precise and Environmentally Clean Stream Discharge Measurements
Hydrology, 2023 Accurate discharge measurement is mandatory for any hydrological study. While the “velocity” measurement method is adapted to laminar flows, the “dilution” method is more appropriate for turbulent streams.Antoine Picard, Florent Barbecot, Gérard Bardoux, Pierre Agrinier, Marina Gillon, José A. Corcho Alvarado, Vincent Schneider, Jean-François Hélie, Frédérick de Oliveira +8 moredoaj +1 more sourceHigh-precision measurements of seawater Pb isotope compositions by double spike thermal ionization mass spectrometry [PDF]
, 2014 A new method for the determination of seawater Pb isotope compositions and concentrations was developed, which combines and optimizes previously published protocols for the separation and isotopic analysis of this element.Bridgestock, L, Paul, M, Rehkämper, M, van DeFlierdt, T, Weiss, D +4 morecore +2 more sourcesEvaluation of diffusive gradients in thin-films using a Diphonix® resin for monitoring dissolved uranium in natural waters [PDF]
, 2015 Commercially available Diphonix® resin (TrisKem International) was evaluated as a receiving phase for use with the diffusive gradients in thin-films (DGT) passive sampler for measuring uranium.Amos, Sean, Burnett, Jonathan L., Fones, Gary R., Mills, Graham A., Turner, Geraldine S. C. +4 morecore +2 more sourcesSyntheses of Labeled Dimethyl Phthalate-D6
Journal of Isotopes, 2014 The synthesis of labeled standard dimethyl phthalate-D6,with CD3OD and benzene anhydride as raw materials by an efficient and no-dilution of isotopic enrichment method was presented, under the catalysis of condensing agent to generate dimethyl phthalate-XU Zhong-jie;LU Wei-jing;SUN Wen;JIANG Zhe;LI Bing-yao;PAN Jiedoaj +1 more sourceShort-lived Nuclei in the Early Solar System: Possible AGB Sources [PDF]
, 2005 (Abridged) We review abundances of short-lived nuclides in the early solar
system (ESS) and the methods used to determine them. We compare them to the
inventory for a uniform galactic production model.Abia, Abia, Alexander, Amari, Amari, Amelin, Amelin, Anders, Anders, Andric, Angulo, Argast, Arlandini, Audouze, Bao, Birck, Birck, Birck, Bizzarro, Black, Blake, Blander, Boothroyd, Boss, Brearley, Burbidge, Burnett, Busso, Busso, Busso, Cameron, Cameron, Cameron, Cameron, Cantelaube, Carlson, Cassen, Cayrel, Chakraborty, Charbonnel, Charbonnel, Chen, Chen, Chen, Chen, Chen, Chen, Chen, Chin, Choi, Choi, Choi, Clayton, Clayton, Clayton, Clayton, Connolly, Cowan, Cuzzi, Cuzzi, Dearborn, Denissenkov, Denissenkov, Desch, Diehl, Draine, Draine, Draine, Ebel, El Goresy, Feigelson, Formicola, Foster, Fowler, Fox, Frost, Frost, G.J. Wasserburg, Gallino, Gallino, Galy, Galy, Gao, Gilroy, Goriely, Goswami, Gounelle, Gray, Gray, Greenstein, Grossman, Grossman, Guan, Göbel, Göpel, Hagee, Harper, Harper, Harper, Harris, Hashizume, Hill, Hill, Hinton, Honda, Hoppe, Hsu, Huss, Huss, Huss, Huss, Huss, Huss, Hutcheon, Hutcheon, Hutcheon, Hutcheon, Iben, Jacobsen, Jacobsen, Jeffery, Jones, K.M. Nollett, Karakas, Karakas, Kelly, Kita, Kleine, Kratz, Krestina, Krot, Käppeler, Lattanzio, Lattanzio, Lee, Lee, Lee, Lee, Lee, Leya, Limongi, Lin, Lin, Lingenfelter, Liu, Lodders, Lodders, Lucatello, Lugaro, Lugaro, Lugaro, Lugmair, Lugmair, Lyons, M. Busso, MacPherson, Marcus, Marhas, Marhas, Marhas, Marhas, Marhas, Marvin, Mauersberger, Mauersberger, Mauersberger, McKeegan, McKeegan, McWilliam, McWilliam, Messenger, Meyer, Meyer, Minster, Mostefaoui, Mostefaoui, Mostefaoui, Mostefaoui, Mowlavi, Murty, Münker, Nakamura, Navon, Nguyen, Nguyen, Nicolussi, Nicolussi, Nicolussi, Nittler, Nittler, Nittler, Nittler, Nittler, Nollett, Nomoto, Nyquist, Nyquist, Ott, Papanastassiou, Podosek, Porcelli, Prantzos, Prinzhofer, Péquignot, Qian, Qian, Qian, Qian, R. Gallino, Rai, Rauscher, Rauscher, Reifarth, Renzini, Reynolds, Rotaru, Rowe, Runkle, Runkle, Russell, Sahijpal, Savina, Schramm, Schramm, Schönbächler, Seeger, Sharp, Sheng, Shu, Shu, Shu, Shukolyukov, Shukolyukov, Simanton, Smith, Sneden, Sneden, Srinivasan, Srinivasan, Srinivasan, Srinivasan, Srinivasan, Stadermann, Stegmann, Stewart, Stirling, Storzer, Straniero, Straniero, Tachibana, Tachibana, Takahashi, Tera, Tera, Thielemann, Thiemens, Thompson, Timmes, Travaglio, Travaglio, Turner, Urey, Urey, Villa, Vockenhuber, Völkening, Wadhwa, Wadhwa, Wasserburg, Wasserburg, Wasserburg, Wasserburg, Wasserburg, Wasserburg, Wasserburg, Wasserburg, Weiss, Whitby, Wilson, Wood, Woodland, Woosley, Woosley, Yin, Yin, Young, Yurimoto, Zinner, Zinner +288 morecore +3 more sourcesThe temperature and chronology of heavy-element synthesis in low-mass
stars [PDF]
, 2015 Roughly half of the heavy elements (atomic mass greater than that of iron)
are believed to be synthesized in the late evolutionary stages of stars with
masses between 0.8 and 8 solar masses. Deep inside the star, nuclei (mainly
iron) capture neutrons and A Jorissen, A. Jorissen, B Gustafsson, B. Plez, CB Stephenson, DA Garcìa-Hernàndez, DL Lambert, E Biémont, E Vassiliadis, F Kupka, F Käppeler, F Käppeler, G Raskin, G Tagliente, G Wallerstein, GJ Mathews, K Takahashi, K-P Schröder, L Siess, L. Siess, M Asplund, MR Savina, O Straniero, O Trippella, P de Laverny, P. Neyskens, PW Merrill, R Alvarez, S Cristallo, S Goriely, S Goriely, S Van Eck, S Van Eck, S Van Eck, S Van Eck, S. Goriely, S. Van Eck, VV Smith, Y Kashiv, ZY Bao +39 morecore +1 more sourceCarbon-rich presolar grains from massive stars : subsolar ¹²C/¹³C and ¹⁴N/¹⁵N ratios and the mystery of ¹⁵N [PDF]
, 2015 Carbon-rich grains with isotopic anomalies compared to the Sun are found in primitive meteorites. They were made by stars, and carry the original stellar nucleosynthesis signature.Fryer, C., Herwig, F., Hirschi, R., Hoppe, P., J. Jordan, C., K. Gibson, B., Pignatari, M., Trappitsch, R., X. Timmes, F., Zinner, E. +9 morecore +3 more sourcesAnalysis of high burnup pressurized water reactor fuel using uranium, plutonium, neodymium, and cesium isotope correlations with burnup
Nuclear Engineering and Technology, 2015 The correlation of the isotopic composition of uranium, plutonium, neodymium, and cesium with the burnup for high burnup pressurized water reactor fuels irradiated in nuclear power reactors has been experimentally investigated.Jung Suk Kim, Young Shin Jeon, Soon Dal Park, Yeong-Keong Ha, Kyuseok Song +4 moredoaj +1 more source