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Paper Citation Record · LEDGER

Dark matter halo properties of the Galactic dwarf satellites: implication for chemo-dynamical evolution of the satellites and a challenge to $\Lambda$CDM

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2206.02821.

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

pith.paper-citation-record.v1
2206.02821 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:33:14.229655Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-13T06:29:25.318917Z

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

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-11T12:33:14.229655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T12:33:14.229655Z digest=sha256:a7c37141d14bd9b5e03d72893b26823cc03061a5bb79e3186c9db0eeb145164b

Observation b459df53-94da-4f67-9f96-56b4cc7bcd1c · inbound

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations cites this paper.

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations Dark matter halo properties of the Galactic dwarf satellites: implication for chemo-dynamical evolution of the satellites and a challenge to $\Lambda$CDM

Reference 9

Resolution
verified exact
local_arxiv, observed 2026-07-13T06:29:25.320626Z

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.

source=arxiv_source observed=2026-07-13T06:28:17.325404Z digest=sha256:79b7e5936709e63257f5b066c03bbb4b50a60f3af5e3a781d601faa83672753f

Observation e715093d-46ea-42a2-aab7-ef04bee4c670 · inbound

Wide binaries in ultra-faint dwarf galaxies as a probe of extended dark objects cites this paper.

Wide binaries in ultra-faint dwarf galaxies as a probe of extended dark objects Dark matter halo properties of the Galactic dwarf satellites: implication for chemo-dynamical evolution of the satellites and a challenge to $\Lambda$CDM

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-01T15:56:21.288447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T15:56:21.288447Z digest=sha256:80507749436156668a9c2fc6f7e0009e77ab88a9c9f2253c970dd16cc66171c8