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Paper Citation Record · LEDGER

A physical model for cosmological simulations of galaxy formation: multi-epoch validation

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.4931.

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

pith.paper-citation-record.v1
1305.4931 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 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T06:58:35.679234Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-20T18:48:53.086151Z

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 ab99858d-2f54-49a3-a352-afae4e5c19cf · inbound

Probing the faint end of simulated galaxy counts at z>3 cites this paper.

Probing the faint end of simulated galaxy counts at z>3 A physical model for cosmological simulations of galaxy formation: multi-epoch validation

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-05-20T18:48:53.087728Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:043b65236239125fba3a086f4a13535fd4089411f73a1eb0998888217812db53

Observation cf4ea603-29fd-4c0c-98ea-ff06f961c226 · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ A physical model for cosmological simulations of galaxy formation: multi-epoch validation

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:35.679234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:35.679234Z digest=sha256:b38d2f6211627140e642601d691f7596910a3836eaf4136d7f56b5528aa0bdc7