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Paper Citation Record · LEDGER

What is the nature of the HESS J1731-347 compact object?

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2306.12326.

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

pith.paper-citation-record.v1
2306.12326 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:36:55.316613Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T23:36:37.377755Z

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 80842641-2443-4861-a754-52845befe1b1 · inbound

Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? cites this paper.

Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars? What is the nature of the HESS J1731-347 compact object?

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-11T18:36:55.316613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:36:55.316613Z digest=sha256:186aa35102c931e9f55a921a81591698c84c09222cecbb1fe71e6bf1443d1a00

Observation d2a73921-d41d-44eb-92ec-a924e5f6eba9 · inbound

Low-frequency observations of low-mass binary systems with neutron star candidates cites this paper.

Low-frequency observations of low-mass binary systems with neutron star candidates What is the nature of the HESS J1731-347 compact object?

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-05T11:20:37.319403Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T11:20:37.319403Z digest=sha256:533211a87215c423c13dc0b6b31ccd437a4b18c1a5bd0dd7f18d3566b3f9e09a

Observation 638db39a-44e9-413d-81a4-cf647e198b03 · 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 What is the nature of the HESS J1731-347 compact object?

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:49:38.968904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:93a79d3130c87faa461ee790ff3a6f52360810866ed2c441e925d3f596839d16

Observation 18aadf95-b985-4464-98cf-251e7c0f5d25 · inbound

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD cites this paper.

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD What is the nature of the HESS J1731-347 compact object?

Reference 110

Resolution
verified exact
arxiv_id, observed 2026-06-30T03:04:15.048834Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-30T01:49:38.961950Z digest=sha256:e1710ac66fad8ea6fda3b03d7a7a58cee2d9cd73438aebd500374c6154231827

Observation fe2b05c4-997f-45a0-ac38-9f0b949b86f6 · 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 What is the nature of the HESS J1731-347 compact object?

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-06-30T15:04:46.628509Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-30T05:13:51.085511Z digest=sha256:308d3cb119bc0dae46fae126558fee0e0f361bed33525201059aea0e0e202da8

Observation efc396a9-311a-4318-bbab-5e87930f5181 · 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 What is the nature of the HESS J1731-347 compact object?

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-04T04:38:45.534150Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:38:45.534150Z digest=sha256:4ca7f5fb1df26c3b88a072172c8c3d0300b79e34c94e8cca4dd9f592018d55b5

Observation 98b11e2e-44ec-4078-836f-f5968cc621da · inbound

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO cites this paper.

Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO What is the nature of the HESS J1731-347 compact object?

Reference 285

Resolution
unresolved
no resolver link, observed 2026-07-12T09:19:35.429829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T09:19:35.429829Z digest=sha256:ed7c7220e53235ed4d32dce3cc26f3e45e359a7a8dab70fab4b96d272c150a01

Observation 03b96e49-d9ec-4dbc-b24c-e67e6c882922 · inbound

Slowly rotating condensate dark stars beyond the mean-field approximation cites this paper.

Slowly rotating condensate dark stars beyond the mean-field approximation What is the nature of the HESS J1731-347 compact object?

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-07-09T23:36:37.378920Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-07-09T23:31:14.212701Z digest=sha256:eae9779f57ee60653156e59c201e60d474380e72eadf15a0ec54085709bfaa40