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Paper Citation Record · LEDGER

RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2208.04332.

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

pith.paper-citation-record.v1
2208.04332 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:46:38.206645Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8ae2735b-aa30-4604-a2e8-9147d3c5660b · inbound

RR Lyrae Stars in Intermediate-age Magellanic Clusters: Membership Probabilities and Delay Time Distribution cites this paper.

RR Lyrae Stars in Intermediate-age Magellanic Clusters: Membership Probabilities and Delay Time Distribution RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-12T17:19:07.362261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T17:19:07.362261Z digest=sha256:fad8e9b5b12c405069ee50149d7f98b209022d6a12edbf0225834671146d6023

Observation a5d48ef6-9670-45dd-8e2b-238fc1faa104 · inbound

A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution cites this paper.

A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-16T00:46:38.206645Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:46:38.206645Z digest=sha256:816300480592bc421a976e3931e97f0b95fd0861b40e116c8c3c413838ee9881