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Paper Citation Record · LEDGER

A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1810.05181.

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

pith.paper-citation-record.v1
1810.05181 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:28:17.218002Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-21T02:13:55.459985Z

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 7c602cf4-84a0-4480-bfa1-f09e20e9b11e · inbound

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Reference 262

Resolution
metadata mismatch
local_arxiv, observed 2026-05-21T02:13:55.462937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6d699b46ff3c4d7229a7fc6dfc19a1ad4c4e5534988da01fca3f44949eadaab0

Observation 55e7a746-9ee3-4277-9e22-3dc25bb3671e · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Reference 240

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:4d2679037a6935b5e1e6c6990b0eb9037eec6a9fef3a61eece4174ef4636ef2e

Observation 8071c353-c6d5-42ec-bb61-ea54cc4250ac · inbound

Exploring the multi-wavelength properties of the high energetic event ZTF20abbiixp/GRB 200524A: from prompt emission to afterglow cites this paper.

Exploring the multi-wavelength properties of the high energetic event ZTF20abbiixp/GRB 200524A: from prompt emission to afterglow A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Reference 182

Resolution
unresolved
no resolver link, observed 2026-08-11T12:28:17.218002Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T12:28:17.218002Z digest=sha256:a53c527a908dd0442c3bd19484e9f6e54275bdbaac221a0cdca4526ad8299fd6