pith. sign in

Integrity report for How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting

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

arXiv:2006.03599 · pith:2020:BCDY7O34BWZI2737NITHX3H2EZ

0Critical
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/BCDY7O34/integrity.json. Pith Number bundles also include signed pith.integrity.v1 events where a Pith Number exists.