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Paper Citation Record · LEDGER

Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.06347.

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

pith.paper-citation-record.v1
2407.06347 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T20:27:08.529132Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T15:04:46.673016Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 d0019c8b-9684-409c-a7ec-c640ef5eca7f · inbound

Oscillatory properties of strange quark stars described by the vector MIT bag model cites this paper.

Oscillatory properties of strange quark stars described by the vector MIT bag model Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-11T20:27:08.529132Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T20:27:08.529132Z digest=sha256:15747175f6d837869b68aa2fe766acf8ffb90d22deaa01acfed9f5519b992b71

Observation 7e22913d-b7fc-415c-9bed-0c88d49835d3 · inbound

Systematic study of the morphology and length of slow stable hybrid star branches cites this paper.

Systematic study of the morphology and length of slow stable hybrid star branches Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?

Reference 44

Resolution
verified exact
arxiv_id, observed 2026-06-30T15:04:46.674303Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-30T05:13:51.085511Z digest=sha256:6fa8a9f70c2b9a83a5228f2f373240ecaa9259371cdce62e7dcbfa7f302818fe

Observation 197d6830-dc2a-4dea-9462-fd78b10679cd · inbound

Systematic study of the morphology and length of slow stable hybrid star branches cites this paper.

Systematic study of the morphology and length of slow stable hybrid star branches Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-04T04:38:46.667736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:38:46.667736Z digest=sha256:3256da9855d6af73ea8c7eec1fa3973c2d7a1133e21b817077789375bbf7750a