Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Is a black hole shadow a reliable test of the no-hair theorem?
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2302.06140.
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 2026-08-07T10:40:41.368495Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T13:51:06.043904Z
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 032bce04-8c52-42a1-a987-0d3877a0cb9c · inbound
Shadow constraints of charged black hole with scalar hair and gravitational waves from extreme mass ratio inspirals cites this paper.
Shadow constraints of charged black hole with scalar hair and gravitational waves from extreme mass ratio inspirals Is a black hole shadow a reliable test of the no-hair theorem?
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:40:41.368495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation baffcb88-4501-4657-b50c-48e291693eb9 · inbound
The shadow and quasinormal modes of the asymptotically flat hairy black holes with a dilaton potential cites this paper.
The shadow and quasinormal modes of the asymptotically flat hairy black holes with a dilaton potential Is a black hole shadow a reliable test of the no-hair theorem?
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T04:52:28.973168Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 379bf468-51d5-4cd3-b53c-18f0f75d2163 · inbound
Reshaping the inner shadow of a Kerr black hole by a torn accretion disk cites this paper.
Reshaping the inner shadow of a Kerr black hole by a torn accretion disk Is a black hole shadow a reliable test of the no-hair theorem?
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T13:51:06.045899Z
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.