Feedback-free starbursts at cosmic dawn - Observable predictions for JWST
A&A, 690 (2024) A108
Published online: 2024-10-03
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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
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EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 ≤ z ≤ 13.5 Using PEARLS and Public JWST Observations
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CEERS: Increasing Scatter along the Star-forming Main Sequence Indicates Early Galaxies Form in Bursts
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Signatures of high-redshift galactic outflows in the thermal Sunyaev Zel’dovich effect
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Simulating High-redshift Galaxies: Enhancing UV Luminosity with Star Formation Efficiency and a Top-heavy IMF
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Age-dating early quiescent galaxies: high star formation efficiency, but consistent with direct, higher-redshift observations
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ALMA observations of super-early galaxies: Attenuation-free model predictions
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Deep Rest-UV JWST/NIRSpec Spectroscopy of Early Galaxies: The Demographics of C iv and N-emitters in the Reionization Era
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Blue monsters at z > 10: Where all their dust has gone
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Physical Origins of Outflowing Cold Clouds in Local Star-forming Dwarf Galaxies
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Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
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The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus
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Dynamics of a Galaxy at z > 10 Explored by JWST Integral Field Spectroscopy: Hints of Rotating Disk Suggesting Weak Feedback
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Probing the Origin of the Star Formation Excess Discovered by JWST through Gamma-Ray Bursts
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Accelerated formation of ultra-massive galaxies in the first billion years
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The Impact of Mass-dependent Stochasticity at Cosmic Dawn
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Redshift-dependent galaxy formation efficiency at z = 5 − 13 in the FirstLight Simulations
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The eventful life of GS-z14-0, the most distant galaxy at redshift z = 14.32
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Witnessing an extreme, highly efficient galaxy formation mode with resolved Lyman-α and Lyman-continuum emission
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