Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Rethinking the 67 Hz QPO in GRS 1915+105: type-C QPOs at the innermost stable circular orbit
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2307.00867.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T03:12:37.477159Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
5
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 365b9a31-a9da-4ef5-8099-02034655e8bc · inbound
Dynamics, Ringdown, and Accretion-Driven Multiple Quasi-Periodic Oscillations of Kerr-Bertotti-Robinson Black Holes cites this paper.
Dynamics, Ringdown, and Accretion-Driven Multiple Quasi-Periodic Oscillations of Kerr-Bertotti-Robinson Black Holes Rethinking the 67 Hz QPO in GRS 1915+105: type-C QPOs at the innermost stable circular orbit
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T03:12:37.477159Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47c2014a-19e9-4631-b312-34b251e923e3 · inbound
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts Rethinking the 67 Hz QPO in GRS 1915+105: type-C QPOs at the innermost stable circular orbit
Reference 64
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T17:28:48.087183Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation a1cd1af9-950e-46d2-8070-33cfffc3858d · inbound
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts cites this paper.
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts Rethinking the 67 Hz QPO in GRS 1915+105: type-C QPOs at the innermost stable circular orbit
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T19:55:01.741996Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 18eeb298-2e15-44c4-be89-fbb8f7904798 · inbound
A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105 cites this paper.
A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105 Rethinking the 67 Hz QPO in GRS 1915+105: type-C QPOs at the innermost stable circular orbit
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:42:15.813504Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.