“…There remains considerable discrepancy between the absolute magnitude of vertical flux estimates derived from 14 C age-model MARs versus 230 Th normalized MARs. However, there is an emerging overall picture in the EEP of: (1) higher Marine Isotope Stage (MIS) 2 C org flux relative to the Holocene with a deglacial peak (Pedersen, 1983;Lyle, 1988;Kienast et al, 2007;Pichevin et al, 2009); (2) lower MIS 2 opal flux relative to the Holocene with a deglacial peak (Bradtmiller et al, 2006(Bradtmiller et al, , 2010Kienast et al, 2006;Warnock et al, 2007;Pichevin et al, 2009;Dubois et al, 2010;Calvo et al, 2011); and (3) constant or lower absolute MIS 2 CaCO 3 flux relative to the Holocene with a slight deglacial peak and better MIS 2 preservation (Loubere, 2004;Loubere and Richaud, 2007;Richaud et al, 2007;Mekik et al, 2012). High MIS 2 C org may be reconciled with low opal if Fe-fertilization decreased the diatom utilization ratio of Si:C and/or increased the solubility of frustules (Watson et al, 2000;Warnock et al, 2007;Pichevin et al, 2009;Dubois et al, 2010).…”