Paper Citation Record · LEDGER

Cosmic web anisotropy is the primary indicator of halo assembly bias

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1903.02007.

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

pith.paper-citation-record.v1
1903.02007 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T11:05:45.565876Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T20:16:21.109603Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 ad422380-e949-49d6-8816-ca71be1d444d · inbound

A Multidimensional Dependence of the Substructure Evolution on the Tidal Coherence cites this paper.

A Multidimensional Dependence of the Substructure Evolution on the Tidal Coherence Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-24T20:16:21.112296Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation bbd7aa2a-7fac-4766-ba2a-1e4aeb434609 · inbound

Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web cites this paper.

Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-03T11:05:45.565876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5c1e453-b4d7-43c2-8f8f-bddfcb6fca97 · inbound

Fast(er)PM and Moving Mesh: JAX-native Geometric Multigrid Methods cites this paper.

Fast(er)PM and Moving Mesh: JAX-native Geometric Multigrid Methods Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 158

Resolution: unresolved; no resolver link, observed 2026-07-14T07:52:28.510358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53567d2f-b129-49ed-9f81-b50788c2b34e · 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 Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T07:53:26.054702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b93969af-b916-487f-9143-aaa3c42cc30c · inbound

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects cites this paper.

Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 21

Resolution: unresolved; no resolver link, observed 2026-07-31T23:49:18.837905Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bddaedbb-a546-4b4b-aa8f-df0bb0bad7e6 · 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 Cosmic web anisotropy is the primary indicator of halo assembly bias

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-01T00:56:15.743180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.