Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.18459.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T04:51:29.840043Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T17:35:32.450152Z
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 77f7d490-27b1-4d4b-b8b1-aac0a7fba784 · inbound
Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR cites this paper.
Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:51:29.840043Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 45cdc94b-3c28-47da-be50-4ec673123df6 · inbound
Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR cites this paper.
Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T17:35:32.456757Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.