Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.01417.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T04:20:40.222994Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T18:15:35.981174Z
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 01ef7809-51e3-43cc-8aca-545e456e94aa · inbound
Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis cites this paper.
Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
Reference 73
- Resolution
- verified exact
- local_arxiv, observed 2026-08-11T18:15:35.987638Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 98404d33-e312-41d6-8e84-f3b0d0a6d9f5 · inbound
SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions cites this paper.
SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions Distinguishing between $\Lambda$CDM and $f(R)$ gravity models using halo ellipticity correlations in simulations
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:20:40.222994Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.