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Paper Citation Record · LEDGER

Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2001.11118.

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

pith.paper-citation-record.v1
2001.11118 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:19:04.093513Z

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 2832c112-805a-46dd-8490-f2a75e601499 · inbound

Constraining Population III stellar demographics with next-generation gravitational-wave observatories cites this paper.

Constraining Population III stellar demographics with next-generation gravitational-wave observatories Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-16T10:19:04.093513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T10:19:04.093513Z digest=sha256:0747b28715623b7ec4acc34de5eab2ffaae22767be6a6d0a18ef5bfe3d0c94c5

Observation 59aface1-43f7-48dd-bb84-b8aee5f5bd4f · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization

Reference 191

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:56.848154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:56.848154Z digest=sha256:2d8da856cf4f18aa78ba436cf5448df91ffa4ab41faf1a928e0cb24fe562b244