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Paper Citation Record · LEDGER

The Relationship Between Simulated Sub-Millimeter and Near-Infrared Images of Sagittarius A* from a Magnetically Arrested Black Hole Accretion Flow

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2404.10982.

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

pith.paper-citation-record.v1
2404.10982 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T17:55:59.050960Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T02:29:22.767127Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0bf3e578-cd80-444b-9010-e8d924303975 · inbound

Constraints on extra charges in dyonic Kerr-Newman-Kasuya-Taub-NUT black hole from the observations of quasi-periodic oscillations cites this paper.

Constraints on extra charges in dyonic Kerr-Newman-Kasuya-Taub-NUT black hole from the observations of quasi-periodic oscillations The Relationship Between Simulated Sub-Millimeter and Near-Infrared Images of Sagittarius A* from a Magnetically Arrested Black Hole Accretion Flow

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-15T17:55:59.050960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T17:55:59.050960Z digest=sha256:343b086814ae5ce8af044881208a49a5257c44c64fb9e01d322eb592bbc3e6bb

Observation 70cd9cd1-751f-4657-86e8-8f8225a2fc03 · inbound

GRMHD and GRRT Simulations of Black Hole Accretion: Flares, Precession, and Complex Spacetimes cites this paper.

GRMHD and GRRT Simulations of Black Hole Accretion: Flares, Precession, and Complex Spacetimes The Relationship Between Simulated Sub-Millimeter and Near-Infrared Images of Sagittarius A* from a Magnetically Arrested Black Hole Accretion Flow

Reference 134

Resolution
verified exact
arxiv_id, observed 2026-07-04T02:29:22.768816Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-06-26T19:45:00.223206Z digest=sha256:bf85100239c0326866a5f9b29274bf66c0c4dc783d1ebe8711af0e36fb43cce8