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Paper Citation Record · LEDGER

Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2008.05991.

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

pith.paper-citation-record.v1
2008.05991 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-01T02:01:27.807230Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T12:25:44.397133Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 db50b7ab-0828-4f0a-a9e5-51d0ad411152 · inbound

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing cites this paper.

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey

Reference 237

Resolution
verified exact
arxiv_id, observed 2026-05-19T09:35:13.101870Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-19T09:35:12.156800Z digest=sha256:d1dae5839e636bc1f285156b5225ef6b985a2291b76a58baadb370dd9c19b93d

Observation 42aef854-2a31-4e7c-a2be-0965d73da9cf · inbound

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics cites this paper.

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-07-01T12:25:44.398579Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-07-01T02:01:27.807230Z digest=sha256:a7baa515e01d2656ccb5c343332709d9159d7a8650a534247492913074cb8df5