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Paper Citation Record · LEDGER

Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2405.17408.

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

pith.paper-citation-record.v1
2405.17408 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-05-18T03:37:40.315677Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T03:40:50.849293Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
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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 7b8587b3-becd-43c2-87e4-d5f80883ccec · inbound

Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity cites this paper.

Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion

Reference 3

Resolution
verified exact
arxiv_id, observed 2026-05-18T03:40:50.852728Z

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=2026-05-18T03:37:40.315677Z digest=sha256:0b27ca9025b70aa75c42369808cc8e7d27babf709ac4f82f602bfefb9d59d30a

Observation f8b48e48-8ef6-4881-8d1f-92987c7254c4 · inbound

General Grad-Shafranov Equation cites this paper.

General Grad-Shafranov Equation Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-05-12T08:01:29.905223Z

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=2026-05-12T01:23:25.135358Z digest=sha256:1f989f09a68817f5287f52665d8fbb3a017addbd41bfa994c4bb86adb2fbd549