Improved astronomical age constraints for the middle Miocene climate transition based on high-resolution stable isotope records from the central Mediterranean Maltese Islands
Article first published online: 10 MAR 2011
Copyright 2011 by the American Geophysical Union.
Volume 26, Issue 1, March 2011
How to Cite
2011), Improved astronomical age constraints for the middle Miocene climate transition based on high-resolution stable isotope records from the central Mediterranean Maltese Islands, Paleoceanography, 26, PA1210, doi:10.1029/2010PA001981., , , , and (
- Issue published online: 10 MAR 2011
- Article first published online: 10 MAR 2011
- Manuscript Accepted: 28 DEC 2010
- Manuscript Revised: 9 SEP 2010
- Manuscript Received: 10 APR 2010
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|palo1674-sup-0001-readme.txt||plain text document||2K||readme.txt|
|palo1674-sup-0002-txts01.doc||Word document||56K||Text S1. The following points are discussed in the text file: (1) construction of the composite sections of Marsalforn and Ras Il Pellegrin, (2) the revised tuning for the Blue Clay Formation, (3) two alternative tuning options for the middle Miocene cooling interval, and (4) a revised tuning of ODP Site 1146.|
|palo1674-sup-0003-fs01.eps||PS document||1196K||Figure S1. Correlation of the Ras Il Pellegrin section (Fomm Ir-Rih Bay, Malta) and the Marsalforn section (Marsalforn, Gozo).|
|palo1674-sup-0004-fs02.eps||PS document||955K||Figure S2. Revised tuning of the basal part of the Blue Clay Formation.|
|palo1674-sup-0005-fs03.eps||PS document||715K||Figure S3. Sedimentation rates across the transition from the Globigerina Limestone Formation to the Blue Clay Formation.|
|palo1674-sup-0006-fs04.eps||PS document||1947K||Figure S4. Stable isotope records of ODP Site 1146 showing the original depth series of Holbourn et al.  and the revised depth records and tuning of this paper.|
|palo1674-sup-0007-fs05.eps||PS document||1940K||Figure S5. Results of cross-spectral comparison (a) between d13C and eccentricity, (b) between d18O and eccentricity, and (c) between d13C and d18O at ODP site 1146.|
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