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Paper Citation Record · LEDGER

Population clustering as a signal for deconfinement in accreting compact stars

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0101002.

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

pith.paper-citation-record.v1
astro-ph/0101002 v3

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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:36:55.279808Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T18:36:55.857846Z

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 92470bad-6f80-4da8-a3c1-2bffcfffe583 · 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? Population clustering as a signal for deconfinement in accreting compact stars

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-08-11T18:36:55.861874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-11T18:36:55.279808Z digest=sha256:140b1ee3600d38bd193ea9bb7fb1638625a8acfbd8ab9ab79e9a0cd0d4c8cbfe

Observation aa0ecc5d-bc98-4eb7-bfa2-b3d1e375859f · inbound

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement cites this paper.

Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement Population clustering as a signal for deconfinement in accreting compact stars

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-03T17:54:36.924145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T17:54:36.924145Z digest=sha256:5d1000fba8302ad7aa8f9f27c9ddd118424115f4ed83cdcc1faaeace82f1e9f1