Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Extending the modeling of the anisotropic galaxy power spectrum to $k = 0.4 \ h\mathrm{Mpc}^{-1}$
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1706.02362.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T22:01:22.490220Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-18T07:01:01.517547Z
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 a946c3b8-8f43-410b-8287-741698adb8a2 · inbound
Simulation budgeting for hybrid effective field theories cites this paper.
Simulation budgeting for hybrid effective field theories Extending the modeling of the anisotropic galaxy power spectrum to $k = 0.4 \ h\mathrm{Mpc}^{-1}$
Reference 92
- Resolution
- verified exact
- local_arxiv, observed 2026-05-18T07:01:01.519340Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation ecf569b1-3413-40fd-ba90-8cdabb080ad8 · inbound
Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors cites this paper.
Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Extending the modeling of the anisotropic galaxy power spectrum to $k = 0.4 \ h\mathrm{Mpc}^{-1}$
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T22:01:22.490220Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.