Paper Citation Record · LEDGER

Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:0711.4126.

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

pith.paper-citation-record.v1
0711.4126 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T05:30:11.156826Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-14T21:09:27.584461Z

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 e410c062-49cc-4e0a-af5e-82d96e97d638 · 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 Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T05:30:11.156826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49863629-d639-41e5-a018-d01f399f9e94 · inbound

Empirical estimates of how massive galaxies can be in {\Lambda}CDM cites this paper.

Empirical estimates of how massive galaxies can be in {\Lambda}CDM Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-05-14T21:09:27.587068Z

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 e4107712-2c51-4d61-89bc-65cc5f8dbba9 · inbound

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses cites this paper.

The dark matter halo mass function in the $\Lambda\mathrm{CDM}$ cosmology at all times and over all scales -- from planetary to galaxy cluster masses Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

Reference 121

Resolution: unresolved; no resolver link, observed 2026-07-11T06:41:50.562143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 206846f1-15e9-454c-9643-7e9b322598f8 · inbound

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures

Reference 150

Resolution: unresolved; no resolver link, observed 2026-07-31T05:29:30.102862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.