Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Critical accretion rates for rapidly growing massive Population III stars
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2306.17223.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:15:08.377330Z
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
1
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 fec123fa-ecbc-405c-9cf2-31329d3d9087 · inbound
The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results cites this paper.
The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results Critical accretion rates for rapidly growing massive Population III stars
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:15:08.377330Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 045499f9-f6db-42f0-abd2-7a4b140b8c01 · 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 Critical accretion rates for rapidly growing massive Population III stars
Reference 144
- Resolution
- verified exact
- arxiv_id, observed 2026-05-08T20:04:08.462922Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.