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. 2017 Nov 29;7:16572. doi: 10.1038/s41598-017-16528-6

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© The Author(s) 2017

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

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Eastern Mediterranean temperature records across TII. LC21 (purple) and ODP967 (orange) G. ruber (a) δ¹⁸O_C and (b,c) Δ₄₇-replicates (shadings correspond to the 95% CI of the 5,000 filtered simulations of the Δ₄₇-replicates). G. ruber Δ₄₇-temperature records from (d) LC21 and (e) ODP967. Dots, thick lines, and shadings in (d,e) as in Fig. 2c. We also show in (a,d) the LC21δ¹⁸O_C and Δ₄₇- temperature late-Holocene values (purple star), respectively. Gaps in the final Δ₄₇-records correspond to intervals where the age uncertainties of the Δ₄₇-replicates do not overlap.