Paper Citation Record · LEDGER

Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:astro-ph/0205322.

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

pith.paper-citation-record.v1
astro-ph/0205322 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.782744Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T02:39:24.268947Z

Reference resolution

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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 215408fc-0d78-452f-a2c5-099d6ceb4d96 · inbound

Can a secluded self-interacting dark sector generate detectable gravitational waves? cites this paper.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.782744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23582092-5259-4d29-a393-15b75f228b1e · inbound

The satellite galaxies of the Milky Way and Andromeda cites this paper.

The satellite galaxies of the Milky Way and Andromeda Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-08T14:18:30.520207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 185d4a0d-cb5e-4b01-8f71-c9a353152622 · inbound

Numerical evolution of self-gravitating halos of self-interacting dark matter cites this paper.

Numerical evolution of self-gravitating halos of self-interacting dark matter Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:20.212834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d615933e-24f8-4bd8-89f0-7a3c5823b8e0 · inbound

Self-Interaction of Super-Resonant Dark Matter cites this paper.

Self-Interaction of Super-Resonant Dark Matter Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-05-21T19:50:33.573405Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 565f7dde-80f8-4019-b896-6cc864ac83a2 · inbound

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM cites this paper.

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-03T06:13:32.272651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9360a20d-0e5f-4bf6-9ba8-93bd2dab3987 · inbound

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations cites this paper.

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 226

Resolution: verified exact; local_arxiv, observed 2026-06-27T16:01:02.043029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 8eafada2-dbf0-441b-ae9b-631881ee0e83 · inbound

Cooling, conduction, compact objects: Gravothermal evolution of dissipative self-interacting dark matter halos cites this paper.

Cooling, conduction, compact objects: Gravothermal evolution of dissipative self-interacting dark matter halos Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 57

Resolution: metadata mismatch; local_arxiv, observed 2026-07-04T02:39:24.270159Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1a54a0a8-739c-4b85-bab3-1404b41a359b · inbound

A Novel Implementation of Self-Interacting Dark Matter in AREPO cites this paper.

A Novel Implementation of Self-Interacting Dark Matter in AREPO Structure and Subhalo Population of Halos in a Self-Interacting Dark Matter Cosmology

Reference 133

Resolution: unresolved; no resolver link, observed 2026-07-11T06:38:02.275303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.