Paper Citation Record · LEDGER

Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2401.15163.

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

pith.paper-citation-record.v1
2401.15163 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:31:40.642821Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T20:16:09.581562Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1a0d9134-7081-43c5-984d-ad691a0db60f · inbound

Implications of modern mass-loss rates for massive stars cites this paper.

Implications of modern mass-loss rates for massive stars Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-06T15:03:21.188062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b89452ee-4d7f-4a10-811a-8921dd465969 · inbound

The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants cites this paper.

The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-05-11T20:16:09.585333Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation f89c3efd-e3ad-4667-8934-edaf91f03aa6 · inbound

White Dwarf Kicks via Episodic Mass Ejection from Red Giant Stars cites this paper.

White Dwarf Kicks via Episodic Mass Ejection from Red Giant Stars Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

Reference 124

Resolution: unresolved; no resolver link, observed 2026-08-15T14:31:40.642821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a03bae7-3696-4c1e-b5f2-284e37427d7d · inbound

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf cites this paper.

JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-14T13:47:23.334455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.