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Integrity report for Ejector and propeller spin-down: How might a superluminous supernova millisecond magnetar become the 6.67 hr pulsar in RCW103

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

arXiv:1608.03149 · pith:2016:NXVMCCGRISGLWBBQ45WX3SYBOP

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Paper page arXiv integrity.json bundle.json

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Findings

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Signed record

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