Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2102.12495.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T19:47:51.839899Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T12:58:07.881074Z
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 1955e853-4536-4459-ac40-5370ea35d730 · 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 New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
Reference 14
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-04T19:47:51.839899Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d335a0fe-e17d-4ab6-8115-d86e0f1b2cc3 · inbound
The first decade of gravitational-wave measurements of black hole spins cites this paper.
The first decade of gravitational-wave measurements of black hole spins New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
Reference 222
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:20:52.377952Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a11f14ef-4bbd-4ad5-9b81-715bb28bd316 · inbound
Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.
Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 New insights on binary black hole formation channels after GWTC-2: young star clusters versus isolated binaries
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T12:58:07.882627Z
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.