@article{df343d6c211c4e1d9b3328e0b69c031a,
title = "Linking the Mediterranean MIS 5 tephra markers to Campi Flegrei (southern Italy) 109–92 ka explosive activity and refining the chronology of MIS 5c-d millennial-scale climate variability",
keywords = "40Ar/39Ar dating, Campi Flegrei, Explosive volcanism, Mediterranean tephrostratigraphy, MIS 5c-d millenial scale variability, Tephra geochemical fingerprinting",
author = "L. Monaco and Palladino, \{D. M.\} and Albert, \{P. G.\} and I. Arienzo and S. Conticelli and \{Di Vito\}, M. and A. Fabbrizio and M. D'Antonio and R. Isaia and Manning, \{C. J.\} and S. Nomade and A. Pereira and P. Petrosino and G. Sottili and R. Sulpizio and G. Zanchetta and B. Giaccio",
note = "Funding Information: R. Jedli{\v c}ka and M. Racek, E. Braschi and A. Orlando, are thanked for providing valuable technical assistance during EPMA analysis at Prague and Florence Universities respectively. Field activities of L.M. were financially supported by “Sapienza” Universit{\`a} di Roma , “Bando di Avvio alla Ricerca”, protocol N° AR120172AD35B81D (responsible: L.M.). G.S. received funding by “Sapienza” University, Fondi di Ateneo-Progetti Medi (protocol N° RM11715C82384428). Financial support was provided by the Competitive fund of the Italian Research Ministry (MUR, PRIN 2017, grant 20177TKBXZ\_003, project “FUTURE, G. Zanchetta, coordinator), issued to MD, BG, DP and GZ. The INGV-OV laboratories have been also financially supported by the EPOS Research Infrastructure through the contribution of the Italian Ministry of University and Research (MUR). P.G.A. is funded through a UK Research and Innovation (UKRI) Future Leaders Fellowship (MR/S035478/1). An earlier version of the manuscript benefited from useful comments from R. Cioni and Sabine Wulf. Ioan Seghedi (IG “SSS” AR) and an anonymous reviewer provided thoughtful and constructive comments that improved the manuscript. Funding Information: R. Jedli?ka and M. Racek, E. Braschi and A. Orlando, are thanked for providing valuable technical assistance during EPMA analysis at Prague and Florence Universities respectively. Field activities of L.M. were financially supported by ?Sapienza? Universit? di Roma, ?Bando di Avvio alla Ricerca?, protocol N? AR120172AD35B81D (responsible: L.M.). G.S. received funding by ?Sapienza? University, Fondi di Ateneo-Progetti Medi (protocol N? RM11715C82384428). Financial support was provided by the Competitive fund of the Italian Research Ministry (MUR, PRIN 2017, grant 20177TKBXZ\_003, project ?FUTURE, G. Zanchetta, coordinator), issued to MD, BG, DP and GZ. The INGV-OV laboratories have been also financially supported by the EPOS Research Infrastructure through the contribution of the Italian Ministry of University and Research (MUR). P.G.A. is funded through a UK Research and Innovation (UKRI) Future Leaders Fellowship (MR/S035478/1). An earlier version of the manuscript benefited from useful comments from R. Cioni and Sabine Wulf. Ioan Seghedi (IG ?SSS? AR) and an anonymous reviewer provided thoughtful and constructive comments that improved the manuscript. Publisher Copyright: {\textcopyright} 2022 Elsevier B.V.",
year = "2022",
month = apr,
doi = "10.1016/j.gloplacha.2022.103785",
language = "English",
volume = "211",
journal = "Global and Planetary Change",
issn = "0921-8181",
publisher = "Elsevier B.V.",
}