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Paper Citation Record · LEDGER

Testing one-loop galaxy bias: cosmological constraints from the power spectrum

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2102.08315.

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

pith.paper-citation-record.v1
2102.08315 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T22:58:53.390127Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-09T22:58:56.510102Z

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 ae164fdb-8d71-4e2a-84b2-4cecb9894f74 · inbound

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions cites this paper.

Boosting galaxy clustering analyses with non-perturbative modelling of redshift-space distortions Testing one-loop galaxy bias: cosmological constraints from the power spectrum

Reference 29

Resolution
verified exact
local_arxiv, observed 2026-08-09T22:58:56.518560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-08-09T22:58:53.390127Z digest=sha256:c44f57d2d096e2f704d8e4cf04dbca6f0cef8d4ddf939ab3bfe3363121d9675e

Observation ef7d69bb-eeea-4f1f-821f-569de52a9a5f · inbound

Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number cites this paper.

Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number Testing one-loop galaxy bias: cosmological constraints from the power spectrum

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-01T07:53:26.695973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:53:26.695973Z digest=sha256:6f13b0c60a67f578a4fdf5277933fa9ec527c72973e9c1c2c0b42c07a2ca7278