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Paper Citation Record · LEDGER

Black Hole - Neutron Star mergers: using kilonovae to constrain the equation of state

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2309.00890.

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

pith.paper-citation-record.v1
2309.00890 v2

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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T14:35:12.505804Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T14:35:12.552652Z

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 3418ee4f-a3a8-45ca-a4a2-c1f5e0afb33d · inbound

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

Explainable autoencoder for neutron star dense matter parameter estimation Black Hole - Neutron Star mergers: using kilonovae to constrain the equation of state

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-08-10T14:35:12.559949Z

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=2026-08-10T14:35:12.505804Z digest=sha256:0ce56f10fbdfa65fc7cc83081270fb0ac8e08f21664efb2cfada4e5c4a8dbec0

Observation a5e94b6b-25e2-4a79-9e02-d07d6ba0180a · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Black Hole - Neutron Star mergers: using kilonovae to constrain the equation of state

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-01T09:55:40.796795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:55:40.796795Z digest=sha256:dcea79822dc4a190c7dd759b8f4befe018cffce98eb614900b81d9d26b60d6b3