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Paper Citation Record · LEDGER

Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1503.01110.

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

pith.paper-citation-record.v1
1503.01110 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 2026-08-12T06:34:41.77262+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T16:14:56.776217Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-19T16:17:38.832988Z

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 456302cf-6c92-48ca-9263-69f490c26c28 · inbound

Simulation-based inference on warm dark matter from HERA forecasts cites this paper.

Simulation-based inference on warm dark matter from HERA forecasts Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-11T16:14:56.776217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ea40c861-1040-42a9-8819-a5f2bed43cd9 · inbound

Abundant Water from Early Supernovae at Cosmic Dawn cites this paper.

Abundant Water from Early Supernovae at Cosmic Dawn Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-10T22:18:28.087353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 015d9db6-c2f2-4d2c-92c8-becc8f035571 · inbound

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe cites this paper.

First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

Reference 278

Resolution
verified exact
local_arxiv, observed 2026-05-14T18:19:23.017177Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:16cccd4e0c9f525d103371eaf6aea6ee8ff202df62bf769e6fd7af96f3612d2b

Observation 0e527197-6412-4598-9649-10b67808065f · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

Reference 164

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:17:38.834518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:335c9fd3b0149f481f0dcfc69d94ffe35014cebd988a0f392a5e0859480bf52f

Observation d748086a-e42f-4807-90e5-66a7e2639512 · 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 Probing The Ultraviolet Luminosity Function of the Earliest Galaxies with the Renaissance Simulations

Reference 170

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:56.753658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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