“…The residence time of Hg is less than ∼2 years in the atmosphere and can be used to represent the transient variation of Hg flux in Earth's history (Mason & Sheu, 2002;Selin, 2009), whereas Mo displays a long residence time in the ocean water (∼400 kyr; Miller et al, 2011). Provided that Hg and Mo are preferentially buried with organic matter and iron sulfide phases (Chappaz et al, 2018;Hlohowskyj et al, 2021;Shen et al, 2020), we propose to use the Hg-Mo relationship as a tool to refine our understanding of Hg sequestration under reducing Not accounting for the samples showing anomalies (n = 15, Figure 3c; n = 11, Figure 3d), Hg displays a high correlation with Mo (r s = 0.86, p < 0.05, n = 73, Figure 3c; r s = 0.86, p < 0.05, n = 20, Figure 3d). For the DBH 15/73 core deposited under a deeper water column, Hg is positively correlated with Mo during the Miaolingian, but shows a negative relationship with Mo during the Stage 10 (Figure 3c).…”