Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2205.10413.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T07:31:58.643897Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 fc79f854-d272-4fb1-a5f2-6df8636da951 · inbound
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.
mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
Reference 105
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T06:20:04.707661Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 245c0aa5-85dc-493d-896a-3da3999a29b4 · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:03.459139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ca21fc16-ec41-43dd-bca4-8e3c31e73327 · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:31:58.643897Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ea0a34aa-450b-4c4d-a212-d06537c4f41b · inbound
Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds cites this paper.
Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:36:23.388113Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.