Paper Citation Record · LEDGER

Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2208.02794.

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

pith.paper-citation-record.v1
2208.02794 v1

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 16 of 16 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T00:30:25.970094Z

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

Reference resolution

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External citation measurements

37
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 15d520e7-d710-45db-a79e-66f7da6069ba · inbound

Exploring the interplay between star formation efficiency and dust in regulating the UV luminosity of early systems in the JWST and ALMA era cites this paper.

Exploring the interplay between star formation efficiency and dust in regulating the UV luminosity of early systems in the JWST and ALMA era Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-23T20:53:25.574055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 4d529ef5-872f-4900-8b20-a11f2bb84d52 · inbound

A novel analysis of contamination in Lyman-break galaxy samples at $\boldsymbol{z\sim6-8}$: spatial correlation with intermediate-redshift galaxies at $\boldsymbol{z\sim1.3-2}$ cites this paper.

A novel analysis of contamination in Lyman-break galaxy samples at $\boldsymbol{z\sim6-8}$: spatial correlation with intermediate-redshift galaxies at $\boldsymbol{z\sim1.3-2}$ Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T23:03:09.903263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dba31514-79f7-4d56-afb1-0a5abbaa56c0 · inbound

The Cosmic Evolution Early Release Science Survey (CEERS) cites this paper.

The Cosmic Evolution Early Release Science Survey (CEERS) Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 136

Resolution: unresolved; no resolver link, observed 2026-08-10T21:46:19.114347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b2734f00-e397-4020-964b-836c47e3f159 · inbound

GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$ cites this paper.

GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$ Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T18:06:29.534218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3859795-3dd7-460e-9bb6-8e06837f6b80 · inbound

Synergising semi-analytical models and hydrodynamical simulations to interpret JWST data from the first billion years cites this paper.

Synergising semi-analytical models and hydrodynamical simulations to interpret JWST data from the first billion years Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-09T11:41:13.937238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5196358-4696-45cf-89a5-eae9b55e604f · inbound

Multi-fidelity emulator for large-scale 21 cm lightcone images: a few-shot transfer learning approach with generative adversarial network cites this paper.

Multi-fidelity emulator for large-scale 21 cm lightcone images: a few-shot transfer learning approach with generative adversarial network Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-08T23:05:15.693226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c076293-44da-4971-aa24-d9bd6438e5a4 · inbound

Dissecting the massive pristine, neutral gas reservoir of a remarkably bright galaxy at z = 14.179 cites this paper.

Dissecting the massive pristine, neutral gas reservoir of a remarkably bright galaxy at z = 14.179 Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-08T17:06:53.359189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2493163a-5f0c-4ef3-ab0c-88baafefd3f9 · inbound

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ cites this paper.

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-06T19:14:42.040949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 682fc2a2-f10f-460f-9c28-5f675cb49bee · inbound

MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe cites this paper.

MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-06T14:12:19.304841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dfd60d2b-8035-42fd-81a3-81b9927f1049 · inbound

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn cites this paper.

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-04T10:26:43.730785Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d612ba0f-479f-4fac-b554-caf04aacb7d6 · 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 Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 2022

Resolution: unresolved; no resolver link, observed 2026-08-04T00:10:13.389076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab15de00-9e2e-40bf-9594-fd96b19058e1 · inbound

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8 cites this paper.

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8 Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-21T15:34:14.766731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 40264c9b-d7bf-4128-9993-daa900b0cd04 · inbound

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA cites this paper.

Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 71

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T05:00:36.713671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation f1b9892a-3c1b-483e-a917-61a6c92bf32e · inbound

Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs cites this paper.

Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-08T23:29:25.471624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0fd51b9e-2cec-4b2c-bc8d-05f5d256f142 · inbound

JWST spectroscopy of galaxies at $z>10$: Damped Ly$\alpha$ absorbers reveal efficient star formation and hidden redshift biases cites this paper.

JWST spectroscopy of galaxies at $z>10$: Damped Ly$\alpha$ absorbers reveal efficient star formation and hidden redshift biases Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 53

Resolution: metadata mismatch; arxiv_id, observed 2026-07-01T02:05:14.567019Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7e96a709-9ca9-4626-824a-5bdd21a9d948 · 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 Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

Reference 142

Resolution: unresolved; no resolver link, observed 2026-08-11T00:30:25.970094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.