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Paper Citation Record · LEDGER

Can the GW190814 secondary component be a bosonic dark matter admixed compact star?

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2110.05538.

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

pith.paper-citation-record.v1
2110.05538 v1

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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T07:26:19.132758Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 a496baef-e5a3-455e-84e7-a0f9cf8043ef · inbound

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach cites this paper.

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach Can the GW190814 secondary component be a bosonic dark matter admixed compact star?

Reference 44

Resolution
unresolved
no resolver link, observed 2026-07-13T05:17:12.889672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T05:17:12.889672Z digest=sha256:8f7b33337e8d5601b2a86ec08d2d5ac403389d1c9e739cf360f408c322e703f5

Observation ed4e2e26-ebe4-4309-b45e-506b3753f093 · inbound

A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects cites this paper.

A story about a tipsy kangaroo: Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects Can the GW190814 secondary component be a bosonic dark matter admixed compact star?

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T07:26:19.132758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:26:19.132758Z digest=sha256:89716f3c1143fd31b2a70c7abf95a9bab1522a32d006e1b144040fe1f6698c08