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Paper Citation Record · LEDGER

Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2003.09663.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2003.09663 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T17:28:11.467640Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-13T05:19:24.916932Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 72462ed0-fd05-4c1a-b685-7e8118b98428 · inbound

Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks cites this paper.

Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-12T15:22:20.346224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T15:22:20.346224Z digest=sha256:d8acd936a0694a8a2f1102d0d277d5a49e6dc7464bb16bd183b24c8e024c520e

Observation 7c689985-cffc-409b-8493-2603a3633972 · inbound

Impact of the returning radiation on X-ray reflection spectroscopy measurements: the case of Galactic black holes cites this paper.

Impact of the returning radiation on X-ray reflection spectroscopy measurements: the case of Galactic black holes Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-10T18:34:38.856570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T18:34:38.856570Z digest=sha256:bb42a60fd10b7b897ae0052909de62f3510807e7e7e37ed8734d6e3f056bf53f

Observation c3e1e867-c45f-4219-8cf5-c65352bc8548 · inbound

Stellar-Mass Black Holes cites this paper.

Stellar-Mass Black Holes Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 125

Resolution
unresolved
no resolver link, observed 2026-08-06T15:40:38.755828Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:40:38.755828Z digest=sha256:890af70f38ab198e9860157769fcb6d1da39523fb9657db5f25649e4ae690696

Observation 07135382-abf0-4867-9a06-30941941ef55 · inbound

Testing General Relativity with Black Holes cites this paper.

Testing General Relativity with Black Holes Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-15T17:28:11.467640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T17:28:11.467640Z digest=sha256:dfd796364691d11580c879b46d105266f08f2deb5cadee26d5f0d916d6d5544e

Observation fb35781e-8c3c-48bc-9baf-9eafb24e3498 · inbound

Testing non-circular black hole spacetime with X-ray reflection cites this paper.

Testing non-circular black hole spacetime with X-ray reflection Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-02T22:32:33.943537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T22:32:33.943537Z digest=sha256:fa658f44bdc871eb8242f4ce49b8b24e5dde8a651ef0b95ef4b20c3a1e38f7e5

Observation ba802930-cad9-496a-a615-9d3f07b89a1d · inbound

Physics and Astrophysics of Black Holes with eXTP cites this paper.

Physics and Astrophysics of Black Holes with eXTP Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-07-13T05:19:24.919119Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-07-13T05:19:16.347394Z digest=sha256:446d76e61cf4368687203d3f56b5bbbd95204144e155793a26118c6419f53b92