Paper Citation Record · LEDGER

The Properties of Cosmic Velocity Fields

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1404.2280.

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

pith.paper-citation-record.v1
1404.2280 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 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:34:12.668924Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T10:39:38.458081Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 2e273342-add0-4291-a4d1-5d99f8bd9e5e · inbound

Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS cites this paper.

Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS The Properties of Cosmic Velocity Fields

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-06T22:34:12.668924Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bcbe6a04-c563-46c9-ada6-94f415efd354 · inbound

Generating Moving Field Initial Conditions with Spatially Varying Boost cites this paper.

Generating Moving Field Initial Conditions with Spatially Varying Boost The Properties of Cosmic Velocity Fields

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:31.922353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7239d3e-7337-43df-adde-e0de82b6c518 · inbound

DISCO-DJ II: a differentiable particle-mesh code for cosmology cites this paper.

DISCO-DJ II: a differentiable particle-mesh code for cosmology The Properties of Cosmic Velocity Fields

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T11:25:30.111233Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28a717b1-58ba-46a3-a6c1-92fa09900152 · inbound

Closing the Observational Gap in Cosmic Dynamics: AI-Enabled Reconstruction of the Universe's Vorticity and Rotational Flow Morphology cites this paper.

Closing the Observational Gap in Cosmic Dynamics: AI-Enabled Reconstruction of the Universe's Vorticity and Rotational Flow Morphology The Properties of Cosmic Velocity Fields

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-04T20:39:20.593716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation a4bea06c-848e-4a86-aa1d-fb6153aba9f7 · inbound

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects cites this paper.

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects The Properties of Cosmic Velocity Fields

Reference 66

Resolution: unresolved; no resolver link, observed 2026-07-31T23:49:22.537709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.