Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1806.01285.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T11:35:56.101450Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-04T19:40:06.489688Z
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 fbd75502-f2e5-43e2-8517-dde1ed047c74 · inbound
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties cites this paper.
Electromagnetic counterparts of black hole-neutron star mergers: dependence on the neutron star properties Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T11:35:56.101450Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3559f058-cb80-43fe-8a1e-4ccab725adba · inbound
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range cites this paper.
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T10:21:19.078899Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 27f7dd8b-87bd-4653-ada4-8feb3544e9e5 · inbound
Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.
Comparing astrophysical models to gravitational-wave data in the observable space Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 57
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T04:37:03.888877Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 7a424b74-f44c-44bc-a5de-f58435b9b7bb · inbound
Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.
Constraints on Line-of-Sight Acceleration from O1-O4 Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 37
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T19:40:06.490959Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 5f6db658-4366-4ed6-a7c4-edb5dbe87f9b · inbound
Constraints on Line-of-Sight Acceleration from O1-O4 cites this paper.
Constraints on Line-of-Sight Acceleration from O1-O4 Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T10:17:28.701972Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0f9a5516-bfa1-4903-98d6-fda4d19ff79f · inbound
Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.
Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:38:52.571510Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.