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Source: paper_references, paper_reference_links, observed 2026-08-03T17:23:04.269220Z
Paper Citation Record · LEDGER
As of 9 August 2026, this Paper Citation Record lists 100 of 135 outbound references and 3 inbound Pith citation observations for arXiv:2512.09980.
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Source: paper_references, paper_reference_links, observed 2026-08-03T17:23:04.269220Z
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Pith citing papers itemized under the disclosed page cap.
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Source: arxiv_reference, observed 2026-07-02T19:47:19.175410Z
100 of 135 outbound references displayed
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings For redshifts z = 5 , 6, 7, and 8 (each treated as a separate observation and inference process), we find a strong degeneracy between the SFE and the string ten- sion
Reference 1
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings The shapes of the posterior distri- butions are flat and constant for string tensions smaller than Gµ ≤ 10−8 andtendstodecreasetowardslarger Gµ
Reference 2
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Here, the UVLFs tend to allow a wider range of values for the various SFE parameters, close to those of priors with and without cosmic strings
Reference 3
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe
Reference 23
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings A Glimpse of the New Redshift Frontier Through Abell S1063
Reference 24
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History From 25 Galaxies at $z_\mathrm{spec}=8.61-13.20$ Confirmed with JWST/NIRSpec
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Unresolved cited work
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UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings Pallottini and A
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Origin of monolithic high-z galaxies and UV luminosity of mergering high-z galaxies in the cosmological model with non-standard spectrum of density perturbations UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings
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