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Paper Citation Record · LEDGER

Kerr-Taub-NUT spacetime to explain the jet power and the radiative efficiency of astrophysical black holes

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2310.10554.

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pith.paper-citation-record.v1
2310.10554 v3

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T04:37:43.117413Z

measured 0 of 1 external citation measurements

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Source: pith, observed 2026-08-06T04:37:44.119436Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

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Pith citing papers

Observation 1991d406-0c51-47f1-9e2e-0c07618a2568 · inbound

Regular Rotating Black Hole: Probing the boundaries of the Radiative Signatures and Jet Power cites this paper.

Regular Rotating Black Hole: Probing the boundaries of the Radiative Signatures and Jet Power Kerr-Taub-NUT spacetime to explain the jet power and the radiative efficiency of astrophysical black holes

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-08-06T04:37:44.123806Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-08-06T04:37:43.117413Z digest=sha256:2985ca88d940c69ded4cf771c21e09d84e28719cbe8fd36c928b3ce2139c49c9