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Paper Citation Record · LEDGER

The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2408.04132.

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

pith.paper-citation-record.v1
2408.04132 v2

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 2026-08-16T06:30:59.297886+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:29:09.014284Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T18:16:22.223912Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

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 6a548d43-0e49-4d30-8c52-0317221b0412 · inbound

A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems cites this paper.

A Survey of General Relativistic Magnetohydrodynamic Models for Black Hole Accretion Systems The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability

Reference 17

Resolution
metadata mismatch
local_arxiv, observed 2026-08-12T17:28:55.754300Z

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=arxiv_source observed=2026-08-12T17:24:17.088493Z digest=sha256:d1d1b2b84d11dc2ea4084e8c55f20849fea3a729fb5987d93cb8fa180f2e5d59

Observation 062937f1-615b-47d3-9089-7000b59949a8 · inbound

Polarimetric Signatures of Bulk Comptonization from within the Plunging Region of Accreting Black Holes cites this paper.

Polarimetric Signatures of Bulk Comptonization from within the Plunging Region of Accreting Black Holes The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-16T11:29:09.014284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:29:09.014284Z digest=sha256:098129884c4df442eb88a47a44f6a03591e3ae3edc3692ba99669e89fb372cab

Observation 4578377b-9b48-4c58-8afd-22d260ae7041 · inbound

The Impact of Plasma Angular Momentum on Magnetically Arrested Flows and Relativistic Jets in Hot Accretion Flows Around Black Holes cites this paper.

The Impact of Plasma Angular Momentum on Magnetically Arrested Flows and Relativistic Jets in Hot Accretion Flows Around Black Holes The 230 GHz Variability of Numerical Models of Sagittarius A* II. The Physical Origins of the Variability

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-16T11:29:05.309732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:29:05.309732Z digest=sha256:f50a7eff6a387bf831741857907976dc20e9a070cff47b6564db3a6e794ccacb