Paper Citation Record · LEDGER

Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:astro-ph/0406247.

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

pith.paper-citation-record.v1
astro-ph/0406247 v2

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T04:27:08.443245Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T02:55:18.944460Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7d9604c7-e726-41eb-89cb-d7d7fe1a52a6 · inbound

Variable gravitational potential of Milky Way analogues in HESTIA suite cites this paper.

Variable gravitational potential of Milky Way analogues in HESTIA suite Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T04:27:08.443245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b80653f1-2a65-4eed-aeef-8aa2992dc628 · inbound

Revisiting the 'Lensing is Low' Problem with UNIONS cites this paper.

Revisiting the 'Lensing is Low' Problem with UNIONS Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:19:07.287695Z

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 abad552b-f54f-4a12-a6b0-4781f9227490 · inbound

Global trends in morphology from massive to dwarf galaxies cites this paper.

Global trends in morphology from massive to dwarf galaxies Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 272

Resolution: verified exact; local_arxiv, observed 2026-07-01T02:55:18.945808Z

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 1468edaa-cebe-4261-87a9-50b0be28e441 · inbound

Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams cites this paper.

Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 116

Resolution: unresolved; no resolver link, observed 2026-07-11T06:35:48.157333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e710e3f0-0582-4a8a-b52c-6e9407427e0d · inbound

Earth rotation turns event timing into a geometric probe of UHE neutrino origin cites this paper.

Earth rotation turns event timing into a geometric probe of UHE neutrino origin Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T09:57:54.291916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df1afc76-6b28-4b30-81ad-42c11fd84022 · 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 Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 61

Resolution: unresolved; no resolver link, observed 2026-07-31T05:29:29.868152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33bbe52c-866d-449f-80de-c43f222bb69f · inbound

Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection cites this paper.

Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-04T01:15:07.142550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.