Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Gravitational-wave luminosity distance in quantum gravity
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1904.00384.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T12:29:21.804143Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-24T19:44:53.281985Z
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 d9b66af3-9cf8-41eb-99ee-55aafc279130 · inbound
Cosmological searches for the neutrino mass scale and mass ordering cites this paper.
Cosmological searches for the neutrino mass scale and mass ordering Gravitational-wave luminosity distance in quantum gravity
Reference 158
- Resolution
- verified exact
- arxiv_id, observed 2026-05-24T19:44:53.284208Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation a8f07d05-f621-469c-9d1a-47f7458ee5ee · inbound
Covariant diffusion and drift of the stochastic GW background with LISA cites this paper.
Covariant diffusion and drift of the stochastic GW background with LISA Gravitational-wave luminosity distance in quantum gravity
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:29:21.804143Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6bdd9428-d2e7-445a-afc7-0ca4e2523902 · inbound
Viscosity in Isotropic Cosmological Backgrounds in General Relativity and Starobinsky Gravity cites this paper.
Viscosity in Isotropic Cosmological Backgrounds in General Relativity and Starobinsky Gravity Gravitational-wave luminosity distance in quantum gravity
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:33:12.846810Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 23130938-ae97-4d82-80f1-e5d864bfa546 · inbound
Hawking area law in quantum gravity cites this paper.
Hawking area law in quantum gravity Gravitational-wave luminosity distance in quantum gravity
Reference 65
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T12:15:22.825718Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation db276e5a-cb55-4a5c-9f27-e43301865137 · inbound
Hawking area law in quantum gravity cites this paper.
Hawking area law in quantum gravity Gravitational-wave luminosity distance in quantum gravity
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T15:57:47.640873Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4b3eac94-a2d7-4b8b-8c8e-a9ca5fa7cd87 · inbound
Noether charges and the first law of thermodynamics for multifractional Schwarzschild black hole in the q-derivative theory cites this paper.
Noether charges and the first law of thermodynamics for multifractional Schwarzschild black hole in the q-derivative theory Gravitational-wave luminosity distance in quantum gravity
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:41:25.204837Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.