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Paper Citation Record · LEDGER

The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1509.02131.

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

pith.paper-citation-record.v1
1509.02131 v2

Coverage vector

measured 0 of 0 reference resolution

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 2026-08-17T06:30:58.91139+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:43:03.789488Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T07:49:38.885201Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 6d9ffd11-4fdb-4b1a-b47c-ea90b7b78f3e · inbound

Explainable autoencoder for neutron star dense matter parameter estimation cites this paper.

Explainable autoencoder for neutron star dense matter parameter estimation The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-10T14:35:12.479549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:35:12.479549Z digest=sha256:f01e90406845eb8a9db54320cacc02b55f6b2e0f410168344c25017f9e919e1d

Observation f33d3d48-9a7c-44ae-bccf-e016bff07f55 · inbound

Radial Oscillations of the HESS J1731-347 Compact Object via the Karmarkar Condition in Gravity cites this paper.

Radial Oscillations of the HESS J1731-347 Compact Object via the Karmarkar Condition in Gravity The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-16T05:43:03.789488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:43:03.789488Z digest=sha256:20ecfb826aa3d356679faf3c65b3b0696aaf73dff7b8d299fa06b99bf4f95781

Observation 15622cde-2d4d-4817-96aa-8fd31400d2f4 · inbound

On the formation of strange quark stars from supernova in compact binaries cites this paper.

On the formation of strange quark stars from supernova in compact binaries The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-06T12:12:25.339035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T12:12:25.339035Z digest=sha256:4e17c1bd8c8926a950aa73f9991434b72f5860b46bbdb13be6fb31877401845c

Observation c929fa37-6f26-4ee2-86c3-21304c8960a9 · inbound

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 49

Resolution
verified exact
local_arxiv, observed 2026-07-04T07:49:38.886455Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:c6527806c7c9b6c728c353627d7e26ad210bf9237420808de5f8bde27bcb036f

Observation 40f05e70-db5b-42fc-9e70-f91ccbc3fb4d · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:06.355493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:06.355493Z digest=sha256:00805736db1f4043931b47008dd9c298634f0f02e0afcb4be3a46cf07dd9dff2