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Paper Citation Record · LEDGER

Indication of Sharp and Strong Phase-Transitions from NICER Observations

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.01619.

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

pith.paper-citation-record.v1
2310.01619 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T14:01:08.737577Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:00:04.482055Z

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 58e825a6-c8b7-4417-bd30-9b41f4fcf474 · inbound

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis cites this paper.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Indication of Sharp and Strong Phase-Transitions from NICER Observations

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T14:01:08.737577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:01:08.737577Z digest=sha256:17ad3e0094c434603bd24b019e0c876c20ad96b31e338f4b8284e3a35048110f

Observation 39818363-7f1a-4de9-b173-50342491d4c7 · 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 Indication of Sharp and Strong Phase-Transitions from NICER Observations

Reference 15

Resolution
verified exact
arxiv_id, observed 2026-07-04T19:00:04.483448Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-25T22:16:36.441357Z digest=sha256:eec59056993f558c584b0464bdf80d8c414bb7e5546f059356df8890ec26d374