Paper Citation Record · LEDGER

Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2407.02674.

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

pith.paper-citation-record.v1
2407.02674 v2

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measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:58:21.917910Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

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External citation measurements

3
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation c26be6ff-f8ce-4970-8620-4c1f1a7109f1 · inbound

No evidence (yet) for increased star-formation efficiency at early times cites this paper.

No evidence (yet) for increased star-formation efficiency at early times Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.917910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4f074cfd-ce78-4610-9706-39b6885f0508 · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-06T18:16:02.998038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e0e6f029-1262-4589-a080-dbcdd789307d · 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 Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 189

Resolution: unresolved; no resolver link, observed 2026-08-04T00:10:33.665096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 18d9f958-e57b-4ab5-a778-265b4c43d01b · inbound

Galaxies at z > 10: {\Lambda}CDM predicts increased Star Formation Efficiency cites this paper.

Galaxies at z > 10: {\Lambda}CDM predicts increased Star Formation Efficiency Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-05-10T04:09:56.623450Z

Source-reported events for the cited work

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Observation 9ba162ad-d0e6-4a8b-a396-0ee965a36075 · inbound

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 143

Resolution: metadata mismatch; local_arxiv, observed 2026-07-09T05:26:02.023487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 79aa6cfb-4786-42b9-a88f-e4e6ac19315d · 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 Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 113

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.506133Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d0b64f6-0a61-4e6c-9064-83b3f3ae81d3 · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 205

Resolution: unresolved; no resolver link, observed 2026-08-01T06:58:52.741004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.