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Paper Citation Record · LEDGER

Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2211.07565.

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

pith.paper-citation-record.v1
2211.07565 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T15:18:35.996758Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

9
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0ea27446-f5d5-41d4-a72b-b4219c457eac · inbound

The constraining power of the Marked Power Spectrum: an analytical study cites this paper.

The constraining power of the Marked Power Spectrum: an analytical study Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-12T15:18:35.996758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T15:18:35.996758Z digest=sha256:ebeaf5f87d76715bb992a960df00ee4ff9ebae677ae9e1440a0c11d2e51da44d

Observation 553f993e-633b-4df5-82c3-8a205c313f6e · inbound

Cosmology with HI Intensity Mapping cites this paper.

Cosmology with HI Intensity Mapping Quijote-PNG: Quasi-maximum likelihood estimation of Primordial Non-Gaussianity in the non-linear halo density field

Reference 200

Resolution
metadata mismatch
local_arxiv, observed 2026-07-12T03:48:27.827025Z

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=arxiv_source observed=2026-07-12T03:43:52.393274Z digest=sha256:bce823d6877a98f084b954119a93afc9e2bbcb3d81e6a009d3b517a5bf1d6456