Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Proof of CMB-driven X-ray brightening of high-z radio galaxies
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2105.03467.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:49:09.551799Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 0266e5f9-2c0e-43be-a840-70b7716eccf0 · inbound
The most extreme high-z radio quasars in the eRASS:1 X-ray survey cites this paper.
The most extreme high-z radio quasars in the eRASS:1 X-ray survey Proof of CMB-driven X-ray brightening of high-z radio galaxies
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:49:09.551799Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.