Integrity report for Orbital migration induced by anisotropic evaporation. Can hot Jupiters form hot Neptunes ?

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

arXiv:1109.2805 · pith:2011:5LWHER65WUDLI4GOC5SY24RGX7

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Paper page arXiv integrity.json bundle.json

Detector runs

Findings

No public integrity findings for this paper.

Signed record

The machine-readable record for this paper lives at /pith/5LWHER65WUDLI4GOC5SY24RGX7/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.