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Paper Citation Record · LEDGER

A Late-Time Radio Flare following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2202.00026.

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

pith.paper-citation-record.v1
2202.00026 v2

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 2026-08-01T13:29:39.401304Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T15:00:39.393646Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 17d23a71-2ea9-4966-9cf4-641d836aa56c · inbound

The Radio Properties of Extreme Coronal Line Emitters: Constraints on the Sub-parsec Environment cites this paper.

The Radio Properties of Extreme Coronal Line Emitters: Constraints on the Sub-parsec Environment A Late-Time Radio Flare following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-07-14T15:00:39.395491Z

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=arxiv_source observed=2026-07-14T14:55:40.318852Z digest=sha256:1e66d60a7c6c115f3c1874cdc023f2479d03306d49953ccfabd1c9933b191105

Observation d0a37847-8ba9-4b91-aa18-6150a6c8bbcb · inbound

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer cites this paper.

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer A Late-Time Radio Flare following a Possible Transition in Accretion State in the Tidal Disruption Event AT 2019azh

Reference 132

Resolution
unresolved
no resolver link, observed 2026-08-01T13:29:39.401304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:29:39.401304Z digest=sha256:933266a88f7b3ac36ba4714b134eab17b472791adba05c4b6c54690728da1ef3