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Paper Citation Record · LEDGER

Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2309.12644.

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

pith.paper-citation-record.v1
2309.12644 v2

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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 2026-08-09T06:31:02.800959+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:49:28.778866Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T13:15:46.610551Z

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Pith citing papers

Observation a760adc9-4a97-45ba-8632-1f0de0186fe1 · inbound

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State cites this paper.

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-06T16:49:28.778866Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 679a1356-68ac-478c-a37b-09984d91c2e6 · inbound

Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure cites this paper.

Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-05-21T23:00:43.690987Z

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.

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Observation 87289bce-aaf9-4fe5-be0e-4041227171e5 · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:21:25.798903Z

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.

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Observation b5f8ad20-fc15-446a-82bb-2587d7d977fd · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-07-01T13:15:46.611854Z

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=pdf_text observed=2026-06-30T23:36:07.718605Z digest=sha256:79577f45e7e2465af4b94716d93663e08238bb0787620239e087e97ebe857972

Observation b58c68f6-7747-47b4-bb9f-cdebccf02d05 · inbound

Paleodetectors for neutrino signals from diverse Galactic stellar collapses cites this paper.

Paleodetectors for neutrino signals from diverse Galactic stellar collapses Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 32

Resolution
unresolved
no resolver link, observed 2026-07-30T19:57:24.339922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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