Pith. sign in

Paper Citation Record · LEDGER

Where do High-Velocity Dark Matter Particles come from in the Milky Way?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2502.17565.

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

pith.paper-citation-record.v1
2502.17565 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T15:29:19.502544Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9384a2ef-a909-45c4-997c-02e83991161b · inbound

Sub-GeV Dark Matter Under Pressure from Direct Detection cites this paper.

Sub-GeV Dark Matter Under Pressure from Direct Detection Where do High-Velocity Dark Matter Particles come from in the Milky Way?

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-06T15:29:19.502544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:29:19.502544Z digest=sha256:4dcc7763bd21eb8d44dbbe0957f2d31903f74cfa42f30929f841908ea5431c0a

Observation 13c795e5-2dfd-478e-9894-d3c2bb447352 · inbound

A Statistical Framework to Identify Kinematically Outlying LMC Globular Clusters and Implications for the LMC's Dark Matter Profile cites this paper.

A Statistical Framework to Identify Kinematically Outlying LMC Globular Clusters and Implications for the LMC's Dark Matter Profile Where do High-Velocity Dark Matter Particles come from in the Milky Way?

Reference 21

Resolution
metadata mismatch
local_arxiv, observed 2026-08-02T18:34:24.114747Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-02T18:31:43.763593Z digest=sha256:643b838bb967f902443ed5851133d522bfc8452300f18519ff843ad1973244aa