Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2005.03955.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:20:27.258579Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T12:08:07.213912Z
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 d5e0d653-6302-4236-9d8d-20cbdb980fa4 · 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 Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:20:27.258579Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c07c3710-3264-43d6-98d0-c88e35d68845 · inbound
Directional dark matter signatures of the Large Magellanic Cloud cites this paper.
Directional dark matter signatures of the Large Magellanic Cloud Predicting the dark matter velocity distribution in galactic structures: tests against hydrodynamic cosmological simulations
Reference 42
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T12:08:07.215209Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.