Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Three Causes of Low-Mass Assembly Bias
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1902.00030.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T16:28:31.371381Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-10T12:00:21.893607Z
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 d830a839-a12f-48d4-aa2c-558f963bbd77 · inbound
The Impact of Galaxy-halo Size Relations on Galaxy Clustering Signals cites this paper.
The Impact of Galaxy-halo Size Relations on Galaxy Clustering Signals The Three Causes of Low-Mass Assembly Bias
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T16:28:31.371381Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6306668d-e8c8-4b82-86cf-e9db86bef901 · inbound
An Improved Fit for Linear Halo Bias at High Redshift cites this paper.
An Improved Fit for Linear Halo Bias at High Redshift The Three Causes of Low-Mass Assembly Bias
Reference 57
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T12:00:21.895528Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation d56674ab-efd8-4909-90f1-edb430d6a5bd · 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 The Three Causes of Low-Mass Assembly Bias
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:53:26.263232Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation afdea8d4-6a5a-42d0-8eec-e905fc621f5e · inbound
Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.
Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models The Three Causes of Low-Mass Assembly Bias
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T05:29:29.372840Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 341ded4b-74c7-4c52-b944-51dcedd29b96 · inbound
Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe cites this paper.
Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe The Three Causes of Low-Mass Assembly Bias
Reference 165
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:56:20.186099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.