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Hain, M., Strecker, M.R., Bookhagen, B., Alonso, R.N., Pingel, H. and ...

Hain, M., Strecker, M.R., Bookhagen, B., Alonso, R.N., Pingel, H. and ...

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TC2006<br />

HAIN ET AL.: SALTA FORELAND FRAGMENTATION<br />

TC2006<br />

Figure 3. Compilation of Neogene stratigraphy <strong>and</strong> chronologic constraints for the three principle intermontane<br />

basins east of the Puna margin. The thicknesses of the formations are not shown to scale as they<br />

have been aligned to a generic time scale that also corresponds to megasequences II to IV of Starck <strong>and</strong><br />

Vergani [1996]. Note that, especially at the Piquete/La Troja contact, diachronous onset of deformation/<br />

syntectonic deposition is implicated. Deposits in the Calchaquí Valley equivalent to the La Troja Formation<br />

have not been investigated herein, but Carrera <strong>and</strong> Muñoz [2008] <strong>and</strong> Salfity et al. [2004] reported Quaternary<br />

strata closely associated with neotectonic compressional structures. Compilation based on the following:<br />

a, Marshall et al. [1983]; b, Grier <strong>and</strong> Dallmeyer [1990]; c, Cout<strong>and</strong> et al. [2006]; d, M. R. <strong>Strecker</strong><br />

(unpublished data, 2001); e, Reynolds et al. [1994]; f, Reynolds et al. [2000]; g, Viramonte et al. [1994]; h,<br />

Viramonte et al. [1984]; i, Malamud et al. [1996]; j, Galli et al. [1996]; k, Grier [1990]; l, Vergani <strong>and</strong><br />

Starck [1988]; m, Gebhard et al. [1974]; n, Gonzalez Villa [2002]; x, this study.<br />

Quaternary deposits [<strong>Hain</strong>, 2008] <strong>and</strong> suggest the adoption<br />

of the name “La Troja Formation.”<br />

3. Methods<br />

3.1. U‐Pb <strong>and</strong> U‐Th Zircon Geochronology<br />

[19] It is important for our assessment of the stratigraphic<br />

record of the poorly exposed, heavily vegetated eastern<br />

sector of the Salta forel<strong>and</strong> that we assign our observations<br />

to the correct formations. For this reason we radiometrically<br />

dated zircons from five volcanic ash samples, one pertaining<br />

to the inferred megafan deposit (Guanaco Formation) <strong>and</strong><br />

four pertaining to the sediments deposited during <strong>and</strong> after<br />

the latest stage of intrabasin deformation (La Troja Formation;<br />

sample sites marked as yellow stars in Figure 2b). U‐Pb<br />

<strong>and</strong> U‐Th zircon ages were obtained using the CAMECA<br />

IMS 1270 ion microprobe at UCLA (Tables 1 <strong>and</strong> 2). Instrument<br />

setup <strong>and</strong> relative sensitivity calibrations for U‐Pb<br />

<strong>and</strong> U‐Th analysis are described by Grove et al. [2003] <strong>and</strong><br />

Schmitt et al. [2006]. U‐Pb age uncertainties estimated from<br />

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