Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2104.10892.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T17:12:21.163112Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T16:35:13.033836Z
Reference resolution
0 of 0 outbound references displayed
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- 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 542160d8-06b4-434b-a24b-fdefd2cf29af · inbound
Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter cites this paper.
Non-Newtonian corrections to radiative viscosity: Israel-Stewart theory as a viscosity limiter Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T17:12:21.163112Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fb8a0ea6-906c-462c-acaf-e51447f45455 · inbound
Blue-tilted Runnings and the JWST Early Galaxy Tension cites this paper.
Blue-tilted Runnings and the JWST Early Galaxy Tension Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T04:44:35.596291Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 707e78dc-70b6-4452-95b3-868b76f9698e · inbound
Blue-tilted Runnings and the JWST Early Galaxy Tension cites this paper.
Blue-tilted Runnings and the JWST Early Galaxy Tension Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
Reference 28
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T16:35:13.035400Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 17b83659-03bc-496e-9d0f-248aec8a9334 · 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 Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
Reference 211
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:10:57.072610Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.