Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Relativistic and wide-angle corrections to galaxy power spectra
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2406.06274.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T19:40:39.064131Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation d873d351-f47d-4ec1-8135-d2231fbb6664 · inbound
Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum cites this paper.
Primordial non-Gaussianity -- the effects of relativistic and wide-angle corrections to the power spectrum Relativistic and wide-angle corrections to galaxy power spectra
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T19:40:39.064131Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5927f5df-88a7-4969-9b36-6a7120d1ecf3 · inbound
Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum cites this paper.
Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum Relativistic and wide-angle corrections to galaxy power spectra
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T22:43:40.857524Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7a86323a-dcfd-4387-9668-92df98d817ec · inbound
The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects cites this paper.
The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects Relativistic and wide-angle corrections to galaxy power spectra
Reference 27
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T14:53:32.127235Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation 61008728-7218-4c2c-b1eb-bfa50f38e6e5 · inbound
The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects cites this paper.
The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects Relativistic and wide-angle corrections to galaxy power spectra
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T18:39:20.634979Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d830bafb-c78d-4cee-9ba1-568c520474e0 · inbound
First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.
First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 Relativistic and wide-angle corrections to galaxy power spectra
Reference 154
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-26T01:38:51.805089Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.