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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 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 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 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T04:37:46.410520Z

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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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 a50d8c19-4bac-4c0d-966b-50f523210b0d · inbound

Generally relativistic description of fast magnetic reconnection induced by thermal electromotive force cites this paper.

Generally relativistic description of fast magnetic reconnection induced by thermal electromotive force Revisiting flares in Sagittarius A* based on general relativistic magnetohydrodynamic numerical simulations of black hole accretion

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-11T04:37:46.410520Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T04:37:46.410520Z digest=sha256:c98492d6e52d01227630d68e1bd8e9351deeaa1af507845d44a9ca3c24dcc850

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-18T03:37:40.315677Z digest=sha256:bfad8e38de18a0c9ad20ff767f59105a790ce4ff50a2237804c6be54bd779db0

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 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-12T01:23:25.135358Z digest=sha256:872097554b53f1d67db62b561faa982a438797dcfeccfd269facb9cee25b9152