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Paper Citation Record · LEDGER

What GW170729's exceptional mass and spin tells us about its family tree

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1903.07813.

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

pith.paper-citation-record.v1
1903.07813 v2

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 2026-08-23T06:30:58.430688+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:55:13.613876Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T07:47:32.783982Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 246e0d47-1bd6-4b2a-9c3b-428632fe7c5a · inbound

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run What GW170729's exceptional mass and spin tells us about its family tree

Reference 251

Resolution
verified exact
arxiv_id, observed 2026-05-16T07:47:32.785712Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-16T07:45:52.838080Z digest=sha256:d62a79d8ef686855364c3c465d556e5517b41df5359f0d344a8a89dbff904143

Observation 35b6437f-9175-4d75-b1bd-de1368b00790 · 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 What GW170729's exceptional mass and spin tells us about its family tree

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-04T19:47:52.062809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:47:52.062809Z digest=sha256:da00b4fab366bf9f30cd86f81ff86dfa6d1dfa54979cd51389bd5bf215523ceb

Observation fbfe6171-08f8-406e-af13-fe9181bd9dc0 · inbound

Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses cites this paper.

Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses What GW170729's exceptional mass and spin tells us about its family tree

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-15T15:55:13.613876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T15:55:13.613876Z digest=sha256:32ffa394a08a715c9f94c20011165286d93d1d71a5afe095ec136780d7db2e9b