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Paper Citation Record · LEDGER

Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2105.02876.

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

pith.paper-citation-record.v1
2105.02876 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T10:38:05.200863Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 96d78989-e678-4b2b-8600-3b9770e08209 · inbound

Low-redshift constraints on structure growth from CMB lensing tomography cites this paper.

Low-redshift constraints on structure growth from CMB lensing tomography Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-04T10:38:05.200863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:38:05.200863Z digest=sha256:2a2168579f41ea942ea14da1e1d11f0edacb12083389b0c6048eea780d3e3da9

Observation f9ea4e81-7b49-4963-bb84-b07113f12917 · 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 Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-01T07:53:21.777394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:53:21.777394Z digest=sha256:56bb74bf7b4d1b6e2a1a2049e05c00ef023b64f985bc238a9045892869a800d0