Pith. sign in

Paper Citation Record · LEDGER

PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2312.12405.

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

pith.paper-citation-record.v1
2312.12405 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T05:30:09.678239Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T18:58:50.528009Z

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 511ac4ce-cf59-4288-9fef-12a310bcda2e · 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 PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-06T05:30:09.678239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T05:30:09.678239Z digest=sha256:75980eb62878286b4b1c888029f03a26cb9fa6d6a01c28762ecfd99425f60148

Observation 0aedea37-eaca-4166-bb21-d852626aeb90 · inbound

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum cites this paper.

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-03T22:43:46.356472Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T22:43:46.356472Z digest=sha256:9000e3f2c1d03e79f57f111a28599edd3b067d294248149ef0a371c4adcc9192

Observation 484f0d29-7dac-4cf5-9265-877a567fa307 · inbound

Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6 cites this paper.

Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6 PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

Reference 68

Resolution
verified exact
arxiv_id, observed 2026-05-10T22:40:49.105143Z

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.

source=pdf_text observed=2026-05-10T19:39:45.988015Z digest=sha256:d40637948bf2e399b75737eae75fa30c2df6d8e2da6de1560189010be5a04008

Observation 8d680350-74a1-43e4-8f43-31029b61428b · inbound

Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe cites this paper.

Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

Reference 43

Resolution
verified exact
arxiv_id, observed 2026-05-11T10:01:04.215116Z

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.

source=pdf_text observed=2026-05-10T15:40:41.819064Z digest=sha256:9f4144897511af34a6d8f7bdcfd3891ec6d845c42ae16a26a7bd5bf300a0194b

Observation 59a32624-55f1-4e1e-8f13-ea04a0293026 · inbound

How I stop worrying about non-universality and $b_\phi$: Constraining local $f_{\rm NL}$ with $b_\phi$ priors from HOD posteriors cites this paper.

How I stop worrying about non-universality and $b_\phi$: Constraining local $f_{\rm NL}$ with $b_\phi$ priors from HOD posteriors PNG-UNITsims: Halo clustering response to primordial non-Gaussianities as a function of mass

Reference 43

Resolution
verified exact
arxiv_id, observed 2026-07-03T18:58:50.529359Z

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.

source=pdf_text observed=2026-07-03T18:57:19.279101Z digest=sha256:c3da6852838efe34e22487723bc28c167ab21d472fc336d34f34bbfe21b8f5b5