Paper Citation Record · LEDGER

Improving cosmological analyses of HI clustering by reducing stochastic noise

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2405.18559.

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

pith.paper-citation-record.v1
2405.18559 v2

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 2026-08-20T06:33:59.587034+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:58:57.450985Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T19:34:14.114332Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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malformed identifier0
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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 358b6432-c072-4087-9642-cabcff0b8cab · inbound

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-12T00:58:57.450985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9bb7fb0-d01e-44c3-aff0-38401457e8be · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T21:30:54.602992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7356cf9-0c12-467b-9f5e-5923dcd187a2 · inbound

Equivalence of the field-level inference and conventional analyses on large scales cites this paper.

Equivalence of the field-level inference and conventional analyses on large scales Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 101

Resolution: verified exact; local_arxiv, observed 2026-08-06T19:34:14.212427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation be2bad19-a3e6-414a-9c87-6c49843fb5dd · inbound

Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics Improving cosmological analyses of HI clustering by reducing stochastic noise

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:35.655663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.