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Paper Citation Record · LEDGER

A massive galaxy that formed its stars at $z \sim 11$

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2308.05606.

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

pith.paper-citation-record.v1
2308.05606 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 2026-08-12T06:34:41.77262+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:45:12.473967Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T00:46:23.810165Z

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 896985fc-92bb-4ce7-94ae-20ecfec37a62 · 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 A massive galaxy that formed its stars at $z \sim 11$

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-11T21:45:12.473967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T21:45:12.473967Z digest=sha256:78e72076f7c4c809ba35d1fd22a4d6e055e29373d43fe3b08aee62473ab3423d

Observation 5d0b08e0-f4be-4423-abc9-0752b1ce51fe · 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 A massive galaxy that formed its stars at $z \sim 11$

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-10T18:44:57.567119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T18:44:57.567119Z digest=sha256:fd6e2a9699a6175cdab117ef6332aa3e976ef28c5a5149147586bd86f998fef2

Observation 3c496568-9601-4e7c-ae1b-7722bc0df653 · 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 A massive galaxy that formed its stars at $z \sim 11$

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-04T00:10:22.428035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T00:10:22.428035Z digest=sha256:2abaeaeb6ff38feb08e754aedd2c8abe7f6de3dc49af8879311a68e4501791ea

Observation 5b1a475b-8a74-4bdb-bb9e-b6e694e0fcf0 · inbound

Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference cites this paper.

Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference A massive galaxy that formed its stars at $z \sim 11$

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-07-02T00:46:23.812697Z

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=2026-06-28T13:17:56.799399Z digest=sha256:12104bf421c8a334e9b1700166cfa4edd633b65c7dd00c25a3800462aba1210f

Observation 548ce085-198b-4a40-bf1b-e8ae7ea9dbd2 · inbound

Satellite quenching by radio jets of central galaxies in galaxy groups cites this paper.

Satellite quenching by radio jets of central galaxies in galaxy groups A massive galaxy that formed its stars at $z \sim 11$

Reference 165

Resolution
unresolved
no resolver link, observed 2026-07-12T06:58:22.474180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T06:58:22.474180Z digest=sha256:fb4528aaf4557243db5ab5689da7b180411e752e5d12d6eb9e4bf29230eb63ec