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Integrity report for Star Clusters in M 31. IV. A Comparative Analysis of Absorption Line Indices in Old M 31 and Milky Way Clusters

A machine-verified record of the checks Pith has run against this paper: detector runs, findings, signed bundle events, and canonical identifiers.

arXiv:1112.2737 · pith:2011:UGLQIIYIADX62PFBEXNGBETVVH

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

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Signed record

The machine-readable record for this paper lives at /pith/UGLQIIYI/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.