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Paper Citation Record · LEDGER

Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2202.11839.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2202.11839 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:20:40.546197Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-06-30T13:54:44.652864Z

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 2220e40f-9b1f-4607-8b2c-8d00d94bdcc7 · inbound

SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions cites this paper.

SHAPE: cosmology with cluster halo intrinsic alignments from subhalo distributions Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-16T04:20:40.546197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2b251f46-55a9-47b1-b8cf-db6a0fc8ea6a · inbound

Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity cites this paper.

Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

Reference 94

Resolution
verified exact
arxiv_id, observed 2026-05-18T17:42:47.147377Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

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Observation f5d64ca0-71c0-428f-92dd-8f60065df525 · inbound

Field-level likelihood for projected fields: Evolved projected fields from initial projected fields cites this paper.

Field-level likelihood for projected fields: Evolved projected fields from initial projected fields Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-04T09:46:16.448856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 99f23f8b-37e3-47fc-bf97-552545f0e0d8 · inbound

Modeling survey-window and integral-constraint effects on PNG in the galaxy power spectrum with light-cone mocks cites this paper.

Modeling survey-window and integral-constraint effects on PNG in the galaxy power spectrum with light-cone mocks Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-06-30T13:54:44.654320Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-30T05:41:24.565390Z digest=sha256:f522e3430cce7e13d6bfbcd8d01f7478908091577d28725d9b895258f3426d38

Observation bd39cde2-9b86-422e-ae0b-be8ab637a22c · 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 Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments

Reference 21

Resolution
unresolved
no resolver link, observed 2026-07-14T06:58:47.359702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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