Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why Must Primordial Non-Gaussianity Be Very Small?
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2104.01953.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T10:25:22.689302Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T13:10:43.200020Z
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 db1100db-7e22-4231-bdf2-7b3d347e9ee5 · inbound
Inflationary background renormalization cites this paper.
Inflationary background renormalization Why Must Primordial Non-Gaussianity Be Very Small?
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T10:25:22.689302Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3388241f-4aab-4d7a-9eba-fed061c8bc52 · inbound
Cosmological constraints on small-scale primordial non-Gaussianity cites this paper.
Cosmological constraints on small-scale primordial non-Gaussianity Why Must Primordial Non-Gaussianity Be Very Small?
Reference 89
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T13:10:43.311233Z
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.
Observation 04d0e268-4218-4f18-853f-53100d294bd4 · inbound
Inflationary trispectrum of gauge fields from scalar and tensor exchanges cites this paper.
Inflationary trispectrum of gauge fields from scalar and tensor exchanges Why Must Primordial Non-Gaussianity Be Very Small?
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T17:12:22.404281Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.