Paper Citation Record · LEDGER

Evaporation: The change from accretion via a thin disk to a coronal flow

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0007091.

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

pith.paper-citation-record.v1
astro-ph/0007091 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T23:53:06.837809Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

12
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bd425d8c-bd81-4e2d-85b0-872b77fb6896 · inbound

A generalized solution for advection-dominated accretion flow, standard disc, and slim disc cites this paper.

A generalized solution for advection-dominated accretion flow, standard disc, and slim disc Evaporation: The change from accretion via a thin disk to a coronal flow

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T23:53:06.837809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6f25204-5a98-4fba-9805-cbc6fdaba38e · inbound

Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies cites this paper.

Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies Evaporation: The change from accretion via a thin disk to a coronal flow

Reference 44

Resolution: metadata mismatch; local_arxiv, observed 2026-05-15T19:56:33.382004Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 81dea54c-263f-4e0e-a989-e488b6d7ec45 · inbound

A narrow Comptonization locus in Seyfert slab coronae: implications for dominant coronal dissipation and reduced feedback cites this paper.

A narrow Comptonization locus in Seyfert slab coronae: implications for dominant coronal dissipation and reduced feedback Evaporation: The change from accretion via a thin disk to a coronal flow

Reference 31

Resolution: metadata mismatch; arxiv_id, observed 2026-05-13T17:40:43.424621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation db750f2f-92fb-4e97-8a2f-6760bc69fb72 · inbound

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 Evaporation: The change from accretion via a thin disk to a coronal flow

Reference 120

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.080463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.