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Paper Citation Record · LEDGER

Minimizing the stochasticity of halos in large-scale structure surveys

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1004.5377.

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

pith.paper-citation-record.v1
1004.5377 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:06:28.059766Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T15:06:29.312728Z

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 273fcac7-1124-4eb0-9b8b-c71f7b6ce4e2 · inbound

Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies cites this paper.

Meta-Calibration of the Cosmic Magnification Coefficient: Toward Unbiased Weak Lensing Reconstruction by Counting Galaxies Minimizing the stochasticity of halos in large-scale structure surveys

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-08-07T15:06:29.316357Z

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.

source=pdf_text observed=2026-08-07T15:06:28.059766Z digest=sha256:10bcd746242240b16fad55a1cdc77e06a72fbaa93e70e894d5a93edbf63d464b

Observation 97564f41-8eac-46c0-9e64-73af29ab6bc0 · inbound

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation cites this paper.

Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation Minimizing the stochasticity of halos in large-scale structure surveys

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-03T23:38:16.380709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T23:38:16.380709Z digest=sha256:27f2e783f2ec2d6682a495662517d29bad1219e2c618426c38d62d9a0baec47a

Observation 9f28bf9f-6caf-48b2-89cd-357f6d43b413 · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Minimizing the stochasticity of halos in large-scale structure surveys

Reference 110

Resolution
unresolved
no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T14:51:12.413085Z digest=sha256:8f85840f2d5a5a10b94ea6418f1f2c3c8d105def2abcee737d8b508dd76d8026