Paper Citation Record · LEDGER

JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2406.18352.

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pith.paper-citation-record.v1
2406.18352 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

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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 JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 33

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Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales cites this paper.

Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 14

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Low dust mass and high star-formation efficiency at $z>12$ from deep ALMA observations cites this paper.

Low dust mass and high star-formation efficiency at $z>12$ from deep ALMA observations JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 44

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Morphological Demographics of Galaxies at $z\sim 10-16$: Log-Normal Size Distribution and Exponential Profiles Consistent with the Disk Formation Scenario cites this paper.

Morphological Demographics of Galaxies at $z\sim 10-16$: Log-Normal Size Distribution and Exponential Profiles Consistent with the Disk Formation Scenario JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 79

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Observation ccd0eaf1-1a8e-4a93-aff9-a69a1292627d · 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 JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 10

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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 JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 34

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Galaxies at z > 10: {\Lambda}CDM predicts increased Star Formation Efficiency cites this paper.

Galaxies at z > 10: {\Lambda}CDM predicts increased Star Formation Efficiency JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 13

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Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology cites this paper.

Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 23

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Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 273

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Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 108

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.753825Z

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Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 139

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Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging cites this paper.

Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

Reference 111

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