Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Shadows of charged rotating black holes: Kerr-Newman versus Kerr-Sen
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2003.14349.
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 2026-08-12T21:39:35.799785Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-25T05:56:40.249771Z
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 6ce53cee-1d3f-44b8-b40b-66dbf8ad1784 · 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 Shadows of charged rotating black holes: Kerr-Newman versus Kerr-Sen
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T21:39:35.799785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e9c4e1d6-3d39-45fb-9390-d5824703f006 · inbound
Constraining Black Hole Parameters in Non-Commutative Geometry using Machine Learning cites this paper.
Constraining Black Hole Parameters in Non-Commutative Geometry using Machine Learning Shadows of charged rotating black holes: Kerr-Newman versus Kerr-Sen
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-05-25T05:56:40.253182Z
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.