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Paper Citation Record · LEDGER

Non-Gaussian tails without stochastic inflation

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2406.02417.

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

pith.paper-citation-record.v1
2406.02417 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T21:23:46.415219Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T02:47:37.756165Z

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 4659e8da-3855-47ae-b983-60c155d20e55 · inbound

Stochastic inflation and non-perturbative power spectrum beyond slow roll cites this paper.

Stochastic inflation and non-perturbative power spectrum beyond slow roll Non-Gaussian tails without stochastic inflation

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-12T21:23:46.415219Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T21:23:46.415219Z digest=sha256:ddc1e6275cc0f7c94b15a875a4e02f087f86ee0b043dccea1307de49c0693025

Observation eefb52df-7a85-4bd1-8024-4e7d76c4e232 · inbound

A consistency relation for induced gravitational wave anisotropies cites this paper.

A consistency relation for induced gravitational wave anisotropies Non-Gaussian tails without stochastic inflation

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-12T21:22:16.244570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T21:22:16.244570Z digest=sha256:c532d16593e49b219affd624eee786e43883021aa2797145b457bf33f3047a2c

Observation 5475a524-03e7-4c12-b9db-539172410aaf · inbound

It\^{o}, Stratonovich, and zoom-in schemes in stochastic inflation cites this paper.

It\^{o}, Stratonovich, and zoom-in schemes in stochastic inflation Non-Gaussian tails without stochastic inflation

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-12T17:37:02.996941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T17:37:02.996941Z digest=sha256:60e5ec0b70e4adb007586bc653b1dbf94620aa0ad0596f07989abd1b37336217

Observation 30278616-a715-4dc0-b8e9-29200bbe7306 · inbound

How Well Do We Know the Scalar-Induced Gravitational Waves? cites this paper.

How Well Do We Know the Scalar-Induced Gravitational Waves? Non-Gaussian tails without stochastic inflation

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-11T19:24:02.038903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T19:24:02.038903Z digest=sha256:332defaf1dfc01e9bb460768ada4a0ad0991330a193d9da8066b3421d6b40eb0

Observation 2318ce79-58b6-4e41-b439-3f40ce855ef2 · inbound

Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA cites this paper.

Reconstructing Primordial Curvature Perturbations via Scalar-Induced Gravitational Waves with LISA Non-Gaussian tails without stochastic inflation

Reference 298

Resolution
unresolved
no resolver link, observed 2026-08-10T18:30:01.120059Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T18:30:01.120059Z digest=sha256:1a51ffc5d5b0b0738f0f464940ab55dc35f28d2bb7cc6d0bd3e9e9989d0fcb70

Observation a4f02320-6008-49e6-9b97-2ddfe4474a63 · inbound

$\delta n$ formalism: A new formulation for the probability density of the curvature perturbation cites this paper.

$\delta n$ formalism: A new formulation for the probability density of the curvature perturbation Non-Gaussian tails without stochastic inflation

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-07T12:38:11.020327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T12:38:11.020327Z digest=sha256:673527b1ea4aa39fa5c3c7262e81bb380914915a00491fdd7e9bd12ed6d48007

Observation ff5b06f3-8154-42ec-a8e9-ca7c31b9279f · inbound

Stochastic scalar-tensor inflation and beyond cites this paper.

Stochastic scalar-tensor inflation and beyond Non-Gaussian tails without stochastic inflation

Reference 71

Resolution
verified exact
arxiv_id, observed 2026-07-02T20:07:21.540497Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-27T21:02:08.476607Z digest=sha256:4c9f0bdea6a7c414a00b4105a556f6682beba05a1321cc2c684e2490d16d160b

Observation 80f13d2b-0391-4be7-a349-37022ea6ab90 · inbound

Stochastic constant-roll inflation beyond the hilltop with the spectral method cites this paper.

Stochastic constant-roll inflation beyond the hilltop with the spectral method Non-Gaussian tails without stochastic inflation

Reference 87

Resolution
verified exact
arxiv_id, observed 2026-07-03T02:47:37.757412Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-27T15:41:12.983843Z digest=sha256:ebf645ef27bac19fbaa4f59cfbe49e2e238df193eabc61999d3e8ead005fd521

Observation f655caef-cbc1-48a8-a76f-66f168bf0324 · inbound

UV artefacts in ultra-slow-roll models of inflation cites this paper.

UV artefacts in ultra-slow-roll models of inflation Non-Gaussian tails without stochastic inflation

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-07-01T17:45:51.283253Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-29T03:21:58.865846Z digest=sha256:784376035a635c0d1311748e2afd61de47cfac09b3b7e723785aa0b4dc416bdb