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Paper Citation Record · LEDGER

The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2406.15237.

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

pith.paper-citation-record.v1
2406.15237 v2

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 2026-08-15T06:32:42.880941+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:54:41.667543Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T18:16:17.926450Z

Reference resolution

0 of 0 outbound references displayed

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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 1784afbc-cd0f-4043-b12b-dc09414ab9eb · inbound

Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data cites this paper.

Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-12T05:04:43.926732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 101f8526-47e2-4902-9971-9fb8859d4588 · inbound

Playground of Lognormal Seminumerical Simulations of~the~Lyman~$\alpha$ Forest: Thermal History of the Intergalactic Medium cites this paper.

Playground of Lognormal Seminumerical Simulations of~the~Lyman~$\alpha$ Forest: Thermal History of the Intergalactic Medium The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-11T14:31:39.652829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:31:39.652829Z digest=sha256:6e1ee809dade8a46cf993df3fdcabdefca56c30c5cf03c7b20888ef9cdc03af6

Observation 5052b774-f8d3-4da7-8777-937e17ac5ac5 · inbound

Temporarily quiescent galaxies at cosmic dawn: probing bursty star formation cites this paper.

Temporarily quiescent galaxies at cosmic dawn: probing bursty star formation The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 69

Resolution
metadata mismatch
local_arxiv, observed 2026-08-10T13:28:37.649994Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-10T13:28:37.017758Z digest=sha256:78d17dc0b767ef6a37090b854559499046787973a56b67dfe4895eedb4d4784e

Observation 77019b1e-b28d-4f3c-a7c1-cd0fb6198fd8 · 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 importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-15T14:54:41.667543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T14:54:41.667543Z digest=sha256:12b602c5316089d367914dc00b5eb9e96cca337439ed25f7468d5317c1c7c60c

Observation aff835df-72d0-416f-b65b-c9c7fdd2a225 · inbound

Constructing X-ray Spectral Models of Galaxies: Varying Contributions from X-ray Binary Populations with Host Galaxy Properties cites this paper.

Constructing X-ray Spectral Models of Galaxies: Varying Contributions from X-ray Binary Populations with Host Galaxy Properties The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 129

Resolution
unresolved
no resolver link, observed 2026-08-14T04:19:01.386955Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:19:01.386955Z digest=sha256:44c9f5d326d1b343c4a32fdc66f8a6d6bee97cbd21e17043d42cfc50e23fd8bb