Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2406.10753.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:20:27.218285Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-19T08:47:12.801254Z
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 f4a56d0b-faaa-41af-951b-e8a3f3ab7fc9 · inbound
Constraints on dark matter self-interaction from velocity distribution function in isolated halos cites this paper.
Constraints on dark matter self-interaction from velocity distribution function in isolated halos Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:20:27.218285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8f9829ac-6ce2-40b6-b872-0d7d047d1bc6 · inbound
Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses cites this paper.
Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
Reference 53
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T08:47:12.805854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 41c4ee63-8fa6-4906-9aaa-4195f92faf69 · inbound
Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations cites this paper.
Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
Reference 49
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:56:22.107869Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 77a11207-262c-42f9-ab75-7dda33ce4631 · 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 Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
Reference 119
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T06:13:41.115538Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 58a57c4c-271b-4c66-ad6e-21d5e9ea5567 · inbound
An Extended Parametric Model for Self-interacting Dark Matter Halos cites this paper.
An Extended Parametric Model for Self-interacting Dark Matter Halos Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
Reference 8
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T15:11:05.256225Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.