Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2109.09741.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:07:31.966307Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T05:06:05.986782Z
Reference resolution
0 of 0 outbound references displayed
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- unresolved0
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- 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 ab8c93d7-4883-49e1-b9ce-a1df215bcc66 · inbound
Machine Learning Techniques for Astrophysics and Cosmology: Photometric Redshifts cites this paper.
Machine Learning Techniques for Astrophysics and Cosmology: Photometric Redshifts Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
Reference 173
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T05:06:05.990555Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 7f162c34-6663-4dad-9fc3-8c8ba2ac352b · inbound
Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation cites this paper.
Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:07:31.966307Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.