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Paper Citation Record · LEDGER

A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2306.07371.

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

pith.paper-citation-record.v1
2306.07371 v4

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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T16:43:48.882408Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9ca4f1d2-d855-48f1-9af1-e4b05813a604 · inbound

Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback? cites this paper.

Can supermassive stars form in protogalaxies due to internal Lyman-Werner feedback? A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-10T16:43:48.882408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T16:43:48.882408Z digest=sha256:39c8e91eb6ed63fefffa7a902ba37463e03412afe97298b8991b6180adfe9875

Observation b72bc7af-77cb-411e-801c-f0256c41c120 · inbound

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations cites this paper.

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories

Reference 28

Resolution
verified exact
arxiv_id, observed 2026-05-08T20:09:06.603065Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-05-08T17:26:07.513278Z digest=sha256:364932f5c725253eb6615c2e8a929186a85a9699a84bb71be88021868b3b4593