Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining the fraction of Compton-thick AGN in the Universe by modelling the diffuse X-ray background spectrum
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1209.5398.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T08:05:16.230513Z
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 0f97ed80-d2a7-4139-a90d-cb1afeb02e0e · inbound
Population synthesis of active galactic nuclei based on the radiation-regulated unification model cites this paper.
Population synthesis of active galactic nuclei based on the radiation-regulated unification model Constraining the fraction of Compton-thick AGN in the Universe by modelling the diffuse X-ray background spectrum
Reference 21
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T22:42:50.139772Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 3e843533-753f-4890-a2fe-28a2df5f80c6 · inbound
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population cites this paper.
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population Constraining the fraction of Compton-thick AGN in the Universe by modelling the diffuse X-ray background spectrum
Reference 12
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T11:28:04.848196Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.