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Paper Citation Record · LEDGER

Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2502.05268.

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

pith.paper-citation-record.v1
2502.05268 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:45:22.467943Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T17:42:47.336518Z

Reference resolution

0 of 0 outbound references displayed

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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 cf3a6a90-8e25-4a55-99af-385a36bc8845 · inbound

Universal Radial Scaling of Large-Scale Black Hole Accretion for Magnetically Arrested And Rocking Accretion Disks cites this paper.

Universal Radial Scaling of Large-Scale Black Hole Accretion for Magnetically Arrested And Rocking Accretion Disks Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-07T12:45:22.467943Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2cae11ff-10cd-4025-ae95-a210dc620ee7 · inbound

Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks cites this paper.

Magnetosonic Waves as a Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-07T04:20:39.434041Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a2cb9659-c685-4487-96e4-09ee4915038a · inbound

Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models cites this paper.

Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Reference 117

Resolution
verified exact
arxiv_id, observed 2026-05-18T17:42:47.339928Z

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.

source=arxiv_source observed=2026-05-18T17:40:44.882670Z digest=sha256:6112104e58a741c933bbafaf58c08ebfc29688f4639da10d6bfde3c38c560a73

Observation b3f26a3d-f6cb-4051-b9ba-eafe02f24506 · inbound

Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN cites this paper.

Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-05-16T17:28:10.157771Z

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.

source=pdf_text observed=2026-05-16T17:25:00.615178Z digest=sha256:915ab229b77acf75867c037076e8aab8285d95c7a230a7dc2d15274b5286b7aa

Observation b5d0a024-2d46-46d7-8554-3f5a47f1bb75 · inbound

How massive and clumpy must a quasar wind be to create emission line blueshifts? cites this paper.

How massive and clumpy must a quasar wind be to create emission line blueshifts? Zooming In On The Multi-Phase Structure of Magnetically-Dominated Quasar Disks: Radiation From Torus to ISCO Across Accretion Rates

Reference 110

Resolution
unresolved
no resolver link, observed 2026-07-31T03:00:27.912686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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