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Paper Citation Record · LEDGER

The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2309.10022.

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

pith.paper-citation-record.v1
2309.10022 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:51:48.411222Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T00:16:16.768632Z

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 035c9eb9-3943-49c1-ad1e-9940c75e37a5 · inbound

The bright, dusty aftermath of giant eruptions & H-rich supernovae. Late interaction of supernova shocks & dusty circumstellar shells cites this paper.

The bright, dusty aftermath of giant eruptions & H-rich supernovae. Late interaction of supernova shocks & dusty circumstellar shells The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-07T20:51:48.411222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T20:51:48.411222Z digest=sha256:77d1ed249144252989e7dd848621bca45d9d01b71ec11a6b6543551889f7f294

Observation 67fabd6f-d510-42cb-8401-8dd31c6bdf5e · inbound

SN 2023ixf: The Closest Supernova of the Decade cites this paper.

SN 2023ixf: The Closest Supernova of the Decade The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-06T18:34:14.365152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:34:14.365152Z digest=sha256:b303449893585e5913beb983f0d67ea43b303fb663ecf2d9009c22372ac932fc

Observation 0124813a-65e7-4d81-a28b-1e9781d7614f · inbound

SN 2023ixf in M101: physical parameters from bolometric light curve modeling cites this paper.

SN 2023ixf in M101: physical parameters from bolometric light curve modeling The Progenitor Star of SN 2023ixf: A Massive Red Supergiant with Enhanced, Episodic Pre-Supernova Mass Loss

Reference 53

Resolution
metadata mismatch
local_arxiv, observed 2026-08-05T22:43:52.928823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-08-05T22:43:50.510640Z digest=sha256:9423a8c5e6c3bee476974096dc64f40778133050e614bf9a945ff5bc4af6408d