Paper Citation Record · LEDGER

The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2304.14469.

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

pith.paper-citation-record.v1
2304.14469 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:11:35.444928Z

measured 1 of 1 external citation measurements

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

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

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External citation measurements

8
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 72592851-f53a-4706-ba5d-fc56a8db403a · inbound

Early Galaxies from Rare Inflationary Processes and JWST Observations cites this paper.

Early Galaxies from Rare Inflationary Processes and JWST Observations The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-08T00:02:53.660503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 688ccf0c-8dcc-493b-a42a-8294dd42e1cd · inbound

Redshift evolution of Lyman continuum escape fraction after JWST cites this paper.

Redshift evolution of Lyman continuum escape fraction after JWST The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T21:11:35.444928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1dd6bd55-9799-4635-abcc-a28f358e1334 · inbound

Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect cites this paper.

Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-06T14:45:35.533215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15abbe76-1608-44e1-85b6-dfadcac97a61 · inbound

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies cites this paper.

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T11:14:20.932196Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd7dd1d4-5532-40ba-8c8a-808d3b9f7b62 · inbound

Probing inflationary features with galaxy ultraviolet luminosity function observables cites this paper.

Probing inflationary features with galaxy ultraviolet luminosity function observables The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T20:12:34.494396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 560cc19c-b425-4556-981d-a1d394629c0d · inbound

Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History cites this paper.

Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-10T11:10:09.591805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 4ed28dc1-a350-4db0-9840-d9ff71a104a2 · inbound

No Blue without Red: Evolutionary Properties of Super-Early Galaxies cites this paper.

No Blue without Red: Evolutionary Properties of Super-Early Galaxies The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-25T05:55:23.675638Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 68f56f09-5313-4d12-b799-9134c58551a9 · 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 galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.494497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c524a1c-c11a-48a9-86a4-7e1dd5498df9 · inbound

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf cites this paper.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T04:20:27.275333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ccf8aa8-e34a-4284-a451-2c3f8ed402e4 · inbound

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models cites this paper.

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 137

Resolution: unresolved; no resolver link, observed 2026-08-11T00:30:25.948741Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.