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Paper Citation Record · LEDGER

Population III star formation: multiple gas phases prevent the use of an equation of state at high densities

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.10730.

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

pith.paper-citation-record.v1
2310.10730 v3

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:44:45.730592Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-07T04:19:31.201530Z

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 561666e5-b150-4656-b7d1-e7ad8cad2dda · inbound

Effect of Magnetic Field on the Accretion Phase of Population III Star Formation cites this paper.

Effect of Magnetic Field on the Accretion Phase of Population III Star Formation Population III star formation: multiple gas phases prevent the use of an equation of state at high densities

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T13:44:45.730592Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T13:44:45.730592Z digest=sha256:893e220d341c5186320da1688ee8a064c1b5ac90c1a6a1ca6802d04f038c9ebc

Observation a7874b07-71f5-4519-9db0-729cafa8e5f3 · inbound

Primordial black holes in cosmological simulations: growth prospects for supermassive black holes cites this paper.

Primordial black holes in cosmological simulations: growth prospects for supermassive black holes Population III star formation: multiple gas phases prevent the use of an equation of state at high densities

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-08-07T04:19:31.254390Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-08-07T04:19:25.552240Z digest=sha256:7ffe98cc0f1bfdea57815d0d24ae37eec9d1d990647af30f94dd12c03acf3f99