Integrity report for Why Supersoft X-ray Fluxes are So Weak in Early-type Galaxies? -- A Clue to Type Ia SN Progenitors --

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

arXiv:1110.0056 · pith:2011:PDQQ3GZPMXCIQ3JNTUSFMPKTJN

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0Advisory

0Detectors run

—Last checked

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/PDQQ3GZPMXCIQ3JNTUSFMPKTJN/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.