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Paper Citation Record · LEDGER

Signatures of mass ratio reversal in gravitational waves from merging binary black holes

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2205.01693.

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

pith.paper-citation-record.v1
2205.01693 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 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.363283Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T22:52:12.842897Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 58d8dc6d-2634-4fb6-950c-84fbbdf2795c · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Signatures of mass ratio reversal in gravitational waves from merging binary black holes

Reference 103

Resolution
verified exact
local_arxiv, observed 2026-08-06T22:52:12.847716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-06T22:52:12.363283Z digest=sha256:57b0d449eef98ec93283990e37bf907a2190924188cc5bb58e2748c7f6c03713

Observation 29a264f1-76ca-40b3-9f52-7af8410ecdc3 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Signatures of mass ratio reversal in gravitational waves from merging binary black holes

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:25.455937Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:25.455937Z digest=sha256:21ae0885fac80f75d2805ba75fcbb51ce2f087e4d42b1f2c920c8ba49a074f23

Observation 89ae2c59-c80f-41d0-a876-6c71c2b8027d · inbound

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations Signatures of mass ratio reversal in gravitational waves from merging binary black holes

Reference 101

Resolution
unresolved
no resolver link, observed 2026-07-31T01:54:12.410906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T01:54:12.410906Z digest=sha256:b79f25aeb4712075d298016c3b61842b2199979f87d13034b5d42b259ec6d7ec