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Paper Citation Record · LEDGER

Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2411.09556.

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

pith.paper-citation-record.v1
2411.09556 v3

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 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:23:30.652773Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c9681352-72fe-4cb2-8323-3e1feb7a5841 · inbound

Survey of Radiative, Two-Temperature Magnetically Arrested Simulations of the Black Hole M87* I: Turbulent Electron Heating cites this paper.

Survey of Radiative, Two-Temperature Magnetically Arrested Simulations of the Black Hole M87* I: Turbulent Electron Heating Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-10T17:23:30.652773Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T17:23:30.652773Z digest=sha256:11ad2ee3f34f9c1cdc511e004d452bea660b71e859812a93df2063461e24fe9c

Observation 2209be6c-cc39-4b1b-9ff4-fb5edb187158 · inbound

Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs cites this paper.

Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*

Reference 36

Resolution
metadata mismatch
arxiv_id, observed 2026-05-12T02:01:14.871725Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-12T01:56:14.015267Z digest=sha256:05abcee90560ec5d2d814bc62a3460e16fbaa27c27b6b61298070ff6e2a75b78

Observation fcc36688-e1df-4e22-aa29-151dd7945eb2 · inbound

Polarization Signatures from GRMHD Simulations of Black Hole Accretion cites this paper.

Polarization Signatures from GRMHD Simulations of Black Hole Accretion Two-temperature treatments in magnetically arrested disk GRMHD simulations more accurately predict light curves of Sagittarius A*

Reference 74

Resolution
verified exact
arxiv_id, observed 2026-05-15T03:08:59.122564Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-15T03:06:24.087052Z digest=sha256:6c64586056692782b73c6a6fbc26c7595ac7c2fea4d119b5c296ecf5cc74aabe