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Paper Citation Record · LEDGER

Limiting masses and radii of neutron stars and their implications

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2009.06441.

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

pith.paper-citation-record.v1
2009.06441 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:28:42.535981Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:00:04.503074Z

Reference resolution

0 of 0 outbound references displayed

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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 b2a5199e-a725-4806-98a2-fbc7c8af6ebb · inbound

The Radius of PSR J0740+6620 from NICER and XMM-Newton Data cites this paper.

The Radius of PSR J0740+6620 from NICER and XMM-Newton Data Limiting masses and radii of neutron stars and their implications

Reference 39

Resolution
verified exact
arxiv_id, observed 2026-05-17T07:01:41.560998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

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Observation b4a1e3fe-c013-4f07-a2a9-c859faaed986 · inbound

Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework cites this paper.

Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework Limiting masses and radii of neutron stars and their implications

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-07T14:28:42.535981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d0f1eab0-c674-43bd-b891-bf319dcc7847 · inbound

Locating the QCD critical point with neutron-star observations cites this paper.

Locating the QCD critical point with neutron-star observations Limiting masses and radii of neutron stars and their implications

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-07T04:40:52.787475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T04:40:52.787475Z digest=sha256:f09b44413bcd6e0a3496915809b48da6556290d0ac85061a83387f44398f7c7d

Observation 2c5e230d-8c29-4155-b274-d253355f9df9 · inbound

Origin of nucleon mass in the light of PSR J0614-3329 with quark-hadron crossover cites this paper.

Origin of nucleon mass in the light of PSR J0614-3329 with quark-hadron crossover Limiting masses and radii of neutron stars and their implications

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-05T11:21:42.017391Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:21:42.017391Z digest=sha256:a868dbf77a96dd86cff32fe9e4c09d0bb04c9246739f30359f7140728a5ef872

Observation 26d16e04-ed18-4329-ad2d-1c5fef35c1c9 · inbound

A quarkyonic matter model cites this paper.

A quarkyonic matter model Limiting masses and radii of neutron stars and their implications

Reference 16

Resolution
verified exact
arxiv_id, observed 2026-07-01T21:16:13.796901Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-28T17:23:06.422687Z digest=sha256:bedb9639118c10b6bd2807a39f444f86b31fa083c858309c52ca22e3d11d7355

Observation 11d6bece-ee0a-4ace-a5da-ea3409cdda9f · inbound

Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements cites this paper.

Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements Limiting masses and radii of neutron stars and their implications

Reference 53

Resolution
verified exact
arxiv_id, observed 2026-07-02T04:06:35.373303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-28T09:24:35.059596Z digest=sha256:287d6efad96486bdc3d6e3c0cf3c4977f9f7d1901a22b1aed09b65331810fa4a

Observation d2f3eeea-32b7-4bb5-b822-5f2cceff4e6d · inbound

Causality alone bounds the maximum radius difference between different-mass neutron stars cites this paper.

Causality alone bounds the maximum radius difference between different-mass neutron stars Limiting masses and radii of neutron stars and their implications

Reference 14

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:00:04.504471Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-25T22:16:36.441357Z digest=sha256:a90c782360e0d9664f44a9579925e1bc6650936f231153a880b6184e1b6a40a8