Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Alleviating the need for exponential evolution of JWST galaxies in 10$^{10} M_{\odot}$ haloes at $z > 10$ by a modified $\Lambda$CDM power spectrum
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2306.04684.
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 2026-08-04T00:10:27.076524Z
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 bf4c8e41-e191-4524-9f87-d282c0295116 · inbound
Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST cites this paper.
Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST Alleviating the need for exponential evolution of JWST galaxies in 10$^{10} M_{\odot}$ haloes at $z > 10$ by a modified $\Lambda$CDM power spectrum
Reference 122
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T00:10:27.076524Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 96c18d74-5cb1-4505-b42a-f8a3b3e9a392 · inbound
Probing inflationary features with galaxy ultraviolet luminosity function observables cites this paper.
Probing inflationary features with galaxy ultraviolet luminosity function observables Alleviating the need for exponential evolution of JWST galaxies in 10$^{10} M_{\odot}$ haloes at $z > 10$ by a modified $\Lambda$CDM power spectrum
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T20:12:34.527099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.