Paper Citation Record · LEDGER

The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2311.00038.

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

pith.paper-citation-record.v1
2311.00038 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:54:12.836726Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d4578d18-08b4-4794-885b-6d1d74a2e987 · inbound

Giants, Supergiants and Hypergiants cites this paper.

Giants, Supergiants and Hypergiants The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-06T18:54:12.836726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a5e536a-ea35-4005-951e-cb41b371bb39 · inbound

Contribution of interstellar objects to local dark matter density cites this paper.

Contribution of interstellar objects to local dark matter density The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 226

Resolution: verified exact; arxiv_id, observed 2026-05-08T17:18:40.013182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a9d795b2-988c-463a-b272-ea7707015e5f · inbound

Charting the Galactic Underworld I: Comprehensive simulations of the kinematics, rates, and demographics of Milky Way black holes cites this paper.

Charting the Galactic Underworld I: Comprehensive simulations of the kinematics, rates, and demographics of Milky Way black holes The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-01T04:30:07.883717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ac464d5d-daa6-4b37-9307-144edfd25f06 · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T20:04:20.792795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0619d943-b926-45fa-b43e-d9a687639bd2 · inbound

Characterization of the variability of the blue supergiant HD 14134 cites this paper.

Characterization of the variability of the blue supergiant HD 14134 The Potential of Asteroseismology to Resolve the Blue Supergiant Problem

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T18:25:19.666455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.