Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Does the shape of the shadow of a black hole depend on motional status of an observer?
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2006.00685.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T21:39:35.749595Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T16:16:06.594556Z
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 a85a3c3b-e0b3-44c5-8823-4d86b38976c8 · inbound
Determining parameters of Kerr-Newman black holes by shadow observation from finite distance and spatial infinity cites this paper.
Determining parameters of Kerr-Newman black holes by shadow observation from finite distance and spatial infinity Does the shape of the shadow of a black hole depend on motional status of an observer?
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T21:39:35.749595Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 144dedec-4de4-49c6-a6ae-5eccfbfdf8e4 · inbound
On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows cites this paper.
On new regular charged black hole solutions: Limiting Curvature Condition, Quasinormal modes and Shadows Does the shape of the shadow of a black hole depend on motional status of an observer?
Reference 131
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T05:25:50.781809Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0ad0dbef-5b59-4024-8c59-0116c0dd420b · inbound
A note on methods for computing the critical curve of Kerr-like black holes cites this paper.
A note on methods for computing the critical curve of Kerr-like black holes Does the shape of the shadow of a black hole depend on motional status of an observer?
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T16:16:06.599142Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.