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Paper Citation Record · LEDGER

Towards a more realistic population of bright spiral galaxies in cosmological simulations

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1304.1559.

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

pith.paper-citation-record.v1
1304.1559 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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:50:05.540341Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 6ceb1ea3-4e12-4d97-87f7-6353e4fd0b82 · inbound

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds cites this paper.

Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds Towards a more realistic population of bright spiral galaxies in cosmological simulations

Reference 75

Resolution
unresolved
no resolver link, observed 2026-07-11T06:21:15.541076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:21:15.541076Z digest=sha256:61335cf06ba6d173bf5390a277a105ca8cdb9e8dbd38476491c8ff805474ef3c

Observation d0cb3a29-28c7-4593-af44-3e029ec539a8 · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime Towards a more realistic population of bright spiral galaxies in cosmological simulations

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-02T03:50:05.540341Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:50:05.540341Z digest=sha256:6fe6c132904a3210fad55b4c7e0b850980b18c34bffa54514e85f0d657f253f8