Paper Citation Record · LEDGER

Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2404.03244.

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

pith.paper-citation-record.v1
2404.03244 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:03:33.654237Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T02:27:10.054658Z

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 3f087009-b930-422a-9c8e-1c49f6c41244 · inbound

A frequentist view on the two-body decaying dark matter model cites this paper.

A frequentist view on the two-body decaying dark matter model Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T14:03:33.654237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4434f0e-23e9-4666-939a-da8395e3e531 · inbound

$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations cites this paper.

$\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-06T05:30:09.581848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fb9e5e9-713a-446d-a9ec-152c2c97e650 · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-16T02:27:10.057457Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 68e3440b-3e5e-45ec-9cde-21fbf74c909c · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 33

Resolution: unresolved; no resolver link, observed 2026-07-14T14:25:37.540627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b766197-f706-4a33-a703-f8b40ea6b541 · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:42.910620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cff78e97-acc8-4c04-aa9e-db6291216555 · inbound

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Scale-dependent local primordial non-Gaussianity as a solution to the $S_8$ tension

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T13:07:47.439644Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.