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Paper Citation Record · LEDGER

Significant uncertainties from calibrating overshooting with eclipsing binary systems

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1808.03523.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1808.03523 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:37:34.816885Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

External citation measurements

36
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation afdd84e5-b3b9-40cb-a39d-061d55359322 · inbound

Shaping the horizontal branch: The role of envelope mass in the evolution of stripped core-helium-burning stars cites this paper.

Shaping the horizontal branch: The role of envelope mass in the evolution of stripped core-helium-burning stars Significant uncertainties from calibrating overshooting with eclipsing binary systems

Reference 108

Resolution
verified exact
local_arxiv, observed 2026-06-27T08:20:44.787154Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b441c19558767636636d53908f4ef9750f4f0a7e8d500eb6140fcd7537927fb1

Observation fd0d35f1-e656-4807-9255-cb28a483a80f · inbound

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems cites this paper.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Significant uncertainties from calibrating overshooting with eclipsing binary systems

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-12T14:37:34.816885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T14:37:34.816885Z digest=sha256:256f862e46f753b82ec75f84c33f7995029585852f947a70c6a3e19b514ce2e0