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Paper Citation Record · LEDGER

The most massive Population III stars

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2302.09763.

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

pith.paper-citation-record.v1
2302.09763 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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T10:26:48.244950Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T11:37:49.022490Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 3fe491db-83b6-4040-8eac-8ce2dbe6b64d · inbound

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn cites this paper.

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn The most massive Population III stars

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-04T10:26:48.244950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:26:48.244950Z digest=sha256:2729ecc481ce548b0128244920e42835a080640adc7c793f249eb7802c369046

Observation f13ba404-5e8b-41cb-ae11-b1dad12bc2d2 · inbound

Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass cites this paper.

Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass The most massive Population III stars

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-16T11:37:49.023892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-05-16T11:34:12.521105Z digest=sha256:b01d4baa3da7ede4f29ef47d408060219db32b100e707b76b7106d9ba82834a1