Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 3 inbound Pith citation observations for arXiv:2401.15163.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T13:47:23.334455Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T20:16:09.581562Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 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 2026-08-14T06:32:32.682623+00:00.
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.