“…The end-Ordovician extinction (444 Ma), end-Permian extinction (252 Ma), end-Triassic extinction (201 Ma), Toarcian OAE (183 Ma), and end-Cretaceous extinction (66 Ma), all feature Hg enrichments that can be correlated on the basis of biostratigraphic or carbon-isotope information across numerous sedimentary sequences spanning multiple regions/continents and both hemispheres (Sanei et al, 2012;Grasby et al, 2013bGrasby et al, , 2016Grasby et al, , 2017Sial et al, 2013Sial et al, , 2014Sial et al, , 2016Sial et al, , 2020Percival et al, 2015Percival et al, , 2017Percival et al, , 2018Font et al, 2016;Thibodeau et al, 2016;Gong et al, 2017;Jones et al, 2017;Fantasia et al, 2018Fantasia et al, , 2019Keller et al, 2018;Wang et al, 2018;Burger et al, 2019;Fendley et al, 2019;Lindström et al, 2019;Meyer et al, 2019;Shen et al, 2019bShen et al, , 2019cSmolarek-Lach et al, 2019;Them et al, 2019). There are also widespread stratigraphic records of the Frasnian-Famennian (372 Ma), Devonian-Carboniferous (359 Ma), and Capitanian (end-Guadalupian, 260 Ma) extinctions, the Valanginian "Weissert" Event (135 Ma), and Paleocene-Eocene Thermal Maximum (PETM, 54 Ma) that feature Hg enrichments (Grasby et al, 2016;Charbonnier et al, 2017, in press;Keller et al, 2018;Kwon et al, 2018;Racki et al, 2018aRacki et al, , 2018bJones et al, 2019;…”