Paper Citation Record · LEDGER

Assembly bias in the clustering of dark matter haloes

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0611921.

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

pith.paper-citation-record.v1
astro-ph/0611921 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 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:12:01.348206Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-12T00:36:17.473008Z

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 23c53612-19dd-4691-9ce0-e3305fa521df · inbound

A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity cites this paper.

A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity Assembly bias in the clustering of dark matter haloes

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-07-04T15:51:57.084669Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 79bbbf0f-2253-4946-912f-2b733d0a6a34 · inbound

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes cites this paper.

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes Assembly bias in the clustering of dark matter haloes

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T18:12:01.348206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d51115a-c3d9-41b8-89bd-a792e7198f37 · inbound

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys cites this paper.

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys Assembly bias in the clustering of dark matter haloes

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T04:21:34.287682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e6236ba-f594-449c-8339-5eeac248917b · inbound

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos cites this paper.

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos Assembly bias in the clustering of dark matter haloes

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-07-04T15:51:57.084669Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation c524d25c-caea-48d5-bcc9-81e4d54ae95c · inbound

The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions cites this paper.

The Environmental Dependence of Halo Intrinsic Alignments: Stronger Signals in Underdense Regions Assembly bias in the clustering of dark matter haloes

Reference 47

Resolution: unresolved; no resolver link, observed 2026-07-14T06:58:47.359702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e0578e2d-26bd-400c-b94a-e43f4ef1fe13 · 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 the clustering of dark matter haloes

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T07:53:19.607340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.