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Paper Citation Record · LEDGER

Gravitational Wave Physics and Astronomy in the nascent era

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2104.02445.

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

pith.paper-citation-record.v1
2104.02445 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T19:47:51.787953Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T05:56:01.601591Z

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 47a7919c-0b11-4197-b67c-581e26ed79bb · inbound

Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors cites this paper.

Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors Gravitational Wave Physics and Astronomy in the nascent era

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:56:01.604122Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-24T05:55:32.580041Z digest=sha256:ca8fbccb055977efb922ce990dc288c0023667edb6f0c882bad35630b53f3eda

Observation 9900c1dd-7320-4d27-9d7c-c62559a24ec7 · inbound

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap cites this paper.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap Gravitational Wave Physics and Astronomy in the nascent era

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-04T19:47:51.787953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:47:51.787953Z digest=sha256:18cf179788580f566985be04e3b7551d9d3d9e49de69d6a96ae0d9627466a2ca