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Paper Citation Record · LEDGER

The 2-point correlation function covariance with fewer mocks

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2306.16332.

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

pith.paper-citation-record.v1
2306.16332 v3

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 2026-08-05T06:32:48.257954+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-30T20:54:13.945175Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T06:00:49.986444Z

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 d558608d-97ce-4875-9d67-08efc5e0b78c · inbound

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars cites this paper.

DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars The 2-point correlation function covariance with fewer mocks

Reference 161

Resolution
verified exact
arxiv_id, observed 2026-05-17T06:00:49.989908Z

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.

source=pdf_text observed=2026-05-17T06:00:49.044220Z digest=sha256:0f598d5f4ace4156f8dbd1e6020dd0e139f99c047f2e6376ba88209d589a2cd2

Observation 516d4529-93d9-4f9b-8366-1b68d654e1e8 · inbound

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics cites this paper.

If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics The 2-point correlation function covariance with fewer mocks

Reference 24

Resolution
verified exact
arxiv_id, observed 2026-05-11T12:31:07.354559Z

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.

source=pdf_text observed=2026-05-10T03:22:25.185479Z digest=sha256:03572b613585fe46e3e9a55fcdcc60c043470b07801a58192674f1897dc9cca8

Observation 664e260a-ca8c-42f3-a0ee-6a8b64ccec43 · inbound

Hermes - Towards an Optimal High-Performance Algorithm for Cosmic Statistics of Large Data Sets cites this paper.

Hermes - Towards an Optimal High-Performance Algorithm for Cosmic Statistics of Large Data Sets The 2-point correlation function covariance with fewer mocks

Reference 147

Resolution
unresolved
no resolver link, observed 2026-07-30T20:54:13.945175Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T20:54:13.945175Z digest=sha256:6c72dbe596e61554c9fa8b46f4ab555ddf9b167ae18cd6e8c36f5ce77cb85b14