Paper Citation Record · LEDGER

Self-Consistent Thermal Accretion Disk Corona Models for Compact Objects: II. Application to Cygnus X-1

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/9705130.

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

pith.paper-citation-record.v1
astro-ph/9705130 v1

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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T17:28:11.397166Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T17:28:12.441738Z

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 1ad8ac18-2379-415d-acfc-cbc8966a1782 · inbound

Probing the Strong Gravity Region of Black Holes with eXTP cites this paper.

Probing the Strong Gravity Region of Black Holes with eXTP Self-Consistent Thermal Accretion Disk Corona Models for Compact Objects: II. Application to Cygnus X-1

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T05:24:43.867720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60bf9aa7-dbb9-4e58-9528-32361e0b732b · inbound

Testing General Relativity with Black Holes cites this paper.

Testing General Relativity with Black Holes Self-Consistent Thermal Accretion Disk Corona Models for Compact Objects: II. Application to Cygnus X-1

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-08-15T17:28:12.445510Z

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.