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Paper Citation Record · LEDGER

Sample Variance Considerations for Cluster Surveys

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0203169.

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

pith.paper-citation-record.v1
astro-ph/0203169 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T12:03:04.963245Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T16:04:53.403677Z

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 30be0819-9ea7-4ed4-a6ca-75c7a5a70ea1 · inbound

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension cites this paper.

Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension Sample Variance Considerations for Cluster Surveys

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-05-17T21:45:18.327535Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-17T21:42:40.737453Z digest=sha256:4d2e6aaae83ca1f40483b4e42fe13520b2845f148a61d51e011b19ab4ff457e6

Observation 1d9cf5ed-7a2e-473b-8c41-af40de16bcf7 · inbound

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference cites this paper.

Cosmology-dependent covariance in galaxy cluster number counts: consequences for parameter inference Sample Variance Considerations for Cluster Surveys

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-06-30T16:04:53.404921Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-30T04:52:09.974573Z digest=sha256:8ba0c3971276ecbcee6a93ec4cf7d8b9fc485eaa5ecf41a7d6e0ee498ac02cf5

Observation fbe20ebd-fafb-47e0-a99d-fc40c148aa9c · inbound

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis cites this paper.

A Gaussian Covariance Matrix for Joint Pre- and Post-Reconstruction Full-Shape Power Spectrum Analysis Sample Variance Considerations for Cluster Surveys

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-08T12:03:04.963245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T12:03:04.963245Z digest=sha256:6e3ee0d47f3d71f082a3407aefc09daacaa590a2efb03d16a854e0bf7b645b40