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Paper Citation Record · LEDGER

Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1711.09907.

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

pith.paper-citation-record.v1
1711.09907 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:21:13.642849Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 f192dc79-8d97-42ef-863d-87d1ed74e587 · inbound

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation cites this paper.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-16T05:21:13.642849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:21:13.642849Z digest=sha256:0e0de75043da8ff1eecea5d5f76396414ef51f39daf63d219d28bcd8c3cf9b84

Observation fd02e005-64b7-428d-a310-79015d56de83 · 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 Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium

Reference 122

Resolution
unresolved
no resolver link, observed 2026-07-30T20:54:13.851448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T20:54:13.851448Z digest=sha256:7602a93b97e439fb7649f817a5b02d1e2df86b93a9cce9d32e82b08019888aa7