Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.10616.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-26T19:28:46.080115Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T02:39:25.249417Z
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 c380fa3f-a3f8-4102-8a8c-f715a256a48e · inbound
Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference cites this paper.
Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T01:12:15.338028Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 885cc131-a7bd-47f9-a282-7e399390fcc3 · inbound
Increasing the sensitivity of full-shape galaxy clustering measurements in configuration-space with three-point statistics cites this paper.
Increasing the sensitivity of full-shape galaxy clustering measurements in configuration-space with three-point statistics Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy
Reference 52
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:39:25.251043Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.