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Paper Citation Record · LEDGER

Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1901.06052.

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

pith.paper-citation-record.v1
1901.06052 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:39:45.189080Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T08:41:25.553442Z

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 35bb7df3-c270-46cf-9d09-e23f844d2aeb · inbound

A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors cites this paper.

A case study of GW190425 for classifying binary neutron star versus binary black hole mergers and constraining asymmetric dark matter with gravitational wave detectors Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-06T18:39:45.189080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:39:45.189080Z digest=sha256:4cf661f71b0779e2be5457d04caf175f3f957935084e8c376cc9eb5926bb9ac5

Observation 1419000a-e0d9-44fa-8d7d-c591526ff217 · inbound

Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers cites this paper.

Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers Can a black hole-neutron star merger explain GW170817, AT2017gfo, GRB170817A?

Reference 80

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:41:25.554695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-07T14:05:21.961266Z digest=sha256:5087523189eb9e092822bb1b8ea80da7a7af26e5d0706e852b4c6506a7f660da