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Paper Citation Record · LEDGER

The impact of mass-dependent stochasticity at cosmic dawn

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2405.13108.

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

pith.paper-citation-record.v1
2405.13108 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:26:10.362562Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T18:44:58.302363Z

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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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 b90dda0c-f8b8-445f-8974-4f3c6e96a3c3 · inbound

BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results cites this paper.

BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results The impact of mass-dependent stochasticity at cosmic dawn

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-11T21:45:12.462611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T21:45:12.462611Z digest=sha256:3c8e42cc29d33d76a545932cab6bbcffda9604b507a50fdbff8806c500dec8a0

Observation d03fee9e-e6fd-4161-8932-19f05e8fd6b2 · inbound

Explaining JWST star formation history at $z \sim 17$ by modifying $\Lambda$CDM cites this paper.

Explaining JWST star formation history at $z \sim 17$ by modifying $\Lambda$CDM The impact of mass-dependent stochasticity at cosmic dawn

Reference 68

Resolution
verified exact
local_arxiv, observed 2026-08-10T18:44:58.307449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-08-10T18:44:57.558130Z digest=sha256:298caba990340540036d065b27ca67f2a094f26bfbf10913565737ac22e4f097

Observation 33e6ca72-3a06-4337-912b-49eda7905b92 · 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 The impact of mass-dependent stochasticity at cosmic dawn

Reference 122

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:56.544215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:56.544215Z digest=sha256:7db76a7ad432fdf426bc2dd773728ea4b7ab9cbf6fb66618c8f58c4e22528af4

Observation 89450011-88c0-48c7-82d6-cce28850a6f4 · inbound

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations cites this paper.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The impact of mass-dependent stochasticity at cosmic dawn

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-15T14:54:41.553962Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T14:54:41.553962Z digest=sha256:80f502b93d5fa31b8b3a9e04bd06fefbf9cbbc0e72ff0d9b5001084bbb393853

Observation cf35a576-3436-4139-9982-6143327a2829 · inbound

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ cites this paper.

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ The impact of mass-dependent stochasticity at cosmic dawn

Reference 199

Resolution
unresolved
no resolver link, observed 2026-08-16T04:26:10.362562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T04:26:10.362562Z digest=sha256:b08ca1f2d5838c44e4c3a8bdcda636ab3d4cd06d28a40298e5be1aeffdec4775