Paper Citation Record · LEDGER

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign

As of 6 August 2026, this Paper Citation Record lists 9 of 9 outbound references and 0 inbound Pith citation observations for arXiv:2604.10287.

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

pith.paper-citation-record.v1
2604.10287 v1

Coverage vector

measured 9 of 9 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-10T15:27:28.843977Z

measured 9 of 9 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 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

9 of 9 outbound references displayed

verified exact2
verified fuzzy2
unresolved2
parse uncertain0
malformed identifier3
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 5ec54ee6-a6ee-4ca0-87c5-a82a32ea29b9 · outbound

This paper cites Revision of two-temperature magnetically arrested flows onto a black hole.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Revision of two-temperature magnetically arrested flows onto a black hole

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-11T10:31:01.472707Z

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.

Observation ddaee31f-ac69-480d-9213-21ed7f5c1fd1 · outbound

This paper cites The visibility amplitude light curves confirm that, unlike Sgr A∗, the other AGN targets exhibit stable flux densities throughout each night of observation.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign The visibility amplitude light curves confirm that, unlike Sgr A∗, the other AGN targets exhibit stable flux densities throughout each night of observation

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T02:12:20.256910Z

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.

Observation 44bfef20-6f22-4570-a71c-eebe73a1dc2f · outbound

This paper cites an unresolved cited work.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-05-18T02:12:20.239464Z

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.

Observation e8fdb80c-5977-4c9a-8286-acd846389f5d · outbound

This paper cites In this appendix we examine in greater detail the behavior of the SF and describe the methodol- ogy employed to estimate PSD slopes and variability timescales.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign In this appendix we examine in greater detail the behavior of the SF and describe the methodol- ogy employed to estimate PSD slopes and variability timescales

Reference 4

Resolution: malformed identifier; raw_fallback, observed 2026-05-18T02:12:20.249441Z

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.

Observation b289f588-4d78-481c-bdc0-999cdbfba320 · outbound

This paper cites This process involved binning the data using a window approximately two times the observational cadence and fitting a spline to the re- sulting light curve.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign This process involved binning the data using a window approximately two times the observational cadence and fitting a spline to the re- sulting light curve

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T02:12:20.253456Z

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.

Observation 45a4463e-9ee9-4441-9bb1-2648692689f8 · outbound

This paper cites an unresolved cited work.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Unresolved cited work

Reference 6

Resolution: verified exact; doi, observed 2026-05-10T21:45:49.170769Z

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.

Observation 52059003-f221-4f99-8271-e4d327fb9b01 · outbound

This paper cites an unresolved cited work.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Unresolved cited work

Reference 7

Resolution: unresolved; raw_fallback, observed 2026-05-18T02:12:20.260166Z

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.

Observation 4e122388-6f03-431d-a4e7-d14f5fe728bc · outbound

This paper cites an unresolved cited work.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign Unresolved cited work

Reference 8

Resolution: malformed identifier; raw_fallback, observed 2026-05-18T02:12:20.242599Z

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.

Observation 0150ff8c-dbd1-4e6a-a49c-8999a9079263 · outbound

This paper cites H.2.Sgr A ∗ accretion rate evolution through the ALMA 2018 observations, estimated from the RM light curve presented in Fig.

Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign H.2.Sgr A ∗ accretion rate evolution through the ALMA 2018 observations, estimated from the RM light curve presented in Fig

Reference 9

Resolution: malformed identifier; raw_fallback, observed 2026-05-18T02:12:20.245979Z

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.

Pith citing papers

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