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Paper Citation Record · LEDGER

The formation of disc galaxies in high resolution moving-mesh cosmological simulations

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.5360.

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

pith.paper-citation-record.v1
1305.5360 v2

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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T22:14:26.547975Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T01:45:14.353338Z

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 a2d81ae1-b8d3-449e-893b-8b044c735afc · inbound

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps cites this paper.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The formation of disc galaxies in high resolution moving-mesh cosmological simulations

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:26.547975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:26.547975Z digest=sha256:a0ab521cb29fa686c194485d4a4246a73b79d66de6a769cee50c26470bf5aa5d

Observation 2ddefbf2-11a2-441b-87c6-69135a6d1354 · inbound

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters cites this paper.

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters The formation of disc galaxies in high resolution moving-mesh cosmological simulations

Reference 73

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:45:14.354503Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:17317bc6bbd6cb840fdb4ff41555dbc8d3abc4bc112c0c3e68fc3174b4b12215