Glorie, S.Thompson, J.Gilbert, S.Souders, A.K.2025-06-022025-06-022025Journal of Analytical Atomic Spectrometry, 2025; 40(5):1394-14020267-94771364-5544https://hdl.handle.net/2440/144867In situ Re–Os geochronology by LA-ICP-MS/MS was previously demonstrated by reacting Os with CH₄ or N₂O reaction gasses. However, for both reactions, a minor proportion of the Re parent isotope also reacts, potentially leading to significant isobaric interferences of ¹⁸⁷Re on ¹⁸⁷Os, especially for young samples with little radiogenic in-growth. Here we present an interlaboratory comparison and compare three reaction gas mixtures (CH₄ + H₂ + He, N₂O and N2O + He) with the aim to robustly date Palaeogene (66–23 Ma) molybdenite from the Bingham Canyon and Henderson deposits. CH₄ mixed with H₂ gas gives the highest sensitivity, while N₂O and He gas buffer Re reaction. On balance, the analytical method involving N₂O + He reaction gas is most suitable for dating Palaeogene molybdenite, resulting in age precision of 2.6% for Bingham and 5.8% for Henderson. For older, >1 Ga molybdenite, CH₄ + H₂ + He may give comparatively better age precision.enThis journal is © The Royal Society of Chemistry 2025In situ Re–Os geochronology of Re-rich Palaeogene molybdenite by LA-ICP-MS/MSIn situ Re–Os geochronology of Re-rich Palaeogene molybdenite by LA-ICP-MS/MS†Journal article10.1039/d5ja00030k737130Glorie, S. [0000-0002-3107-9028]Gilbert, S. [0000-0003-3259-7983]