Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:astro-ph/0107431.
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 2026-08-15T18:18:53.789540Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-27T11:30:52.858865Z
Reference resolution
0 of 0 outbound references displayed
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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 e57919aa-fc3b-4183-81d4-209129de98fc · inbound
Quadratic estimators for unwindowed power spectrum of galaxy-galaxy weak lensing and its application to $P_{\rm gm}(k)$ estimation cites this paper.
Quadratic estimators for unwindowed power spectrum of galaxy-galaxy weak lensing and its application to $P_{\rm gm}(k)$ estimation Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T18:18:53.789540Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 74c7aec2-a5b0-4e1f-9e2f-f3ff54b0ba43 · inbound
Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity cites this paper.
Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 99
- Resolution
- verified exact
- local_arxiv, observed 2026-05-18T17:42:47.239943Z
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 209220be-4f43-4e3d-93ec-14a6ca40dabf · inbound
Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology cites this paper.
Modeling Redshift Uncertainties in Roman Weak Lensing Cosmology Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T03:05:15.331242Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ebd304b5-1abc-4f63-870d-4472838e3d84 · inbound
Modeling the impact of filter-substrate refraction in the Roman point spread function cites this paper.
Modeling the impact of filter-substrate refraction in the Roman point spread function Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T11:30:52.860255Z
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 b4744c43-9618-4593-8949-6f06b3b53a30 · inbound
The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions cites this paper.
The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T06:58:47.359702Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2367a89d-7c8e-42ad-8bff-3b0caf933c4a · inbound
An optimal quadratic estimator for window-free cosmic shear power spectra cites this paper.
An optimal quadratic estimator for window-free cosmic shear power spectra Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:37:24.216919Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1e009aac-dee0-4ac7-a963-1f7de83c952f · 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 Shapes and Shears, Stars and Smears: Optimal Measurements for Weak Lensing
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:07:32.219772Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.