Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2106.14713.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T00:58:57.437169Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T21:30:56.891367Z
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 bb08dbfa-6070-44be-ad2a-3ee7d5e9c37b · inbound
The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.
The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T00:58:57.437169Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1b0303b6-899e-4907-b62e-e77ce9613cd5 · inbound
Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.
Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
Reference 63
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T21:30:56.904024Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 49e0c266-3a2a-417d-b504-7a1155ee1c85 · 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 Assembly bias in quadratic bias parameters of dark matter halos from forward modeling
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:53:25.802485Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.