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Paper Citation Record · LEDGER

Initial-final mass relation from white dwarfs within 40 pc

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.15410.

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

pith.paper-citation-record.v1
2310.15410 v1

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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T21:05:50.564481Z

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
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

40
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4728de8e-7f5b-4d9b-b286-c0af3eb85909 · inbound

Comparison of methods used to derive the Galactic star formation history from white dwarf samples cites this paper.

Comparison of methods used to derive the Galactic star formation history from white dwarf samples Initial-final mass relation from white dwarfs within 40 pc

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-07T21:05:50.564481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T21:05:50.564481Z digest=sha256:426d29f087531113bd8af4cb954c4d0195cb5f853407aa0ee9ff1b8d84da22b9

Observation 3ae1edc7-f3c6-4619-a3d4-9b37106b60f6 · inbound

White dwarfs within 13 pc: Insights from ultraviolet spectroscopy cites this paper.

White dwarfs within 13 pc: Insights from ultraviolet spectroscopy Initial-final mass relation from white dwarfs within 40 pc

Reference 135

Resolution
verified exact
local_arxiv, observed 2026-07-08T08:44:45.118467Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d3586e48fd00c48d7e2bca739b66273030626604f4abffd222e1126586e2d363