SERENADE III: Insight into the Origin of the High Dust Temperature and High [O III]/[C II] Ratio at z 6
astro-ph.GA
Submitted: 2026-08-27
Updated: 2026-08-27
Terminology
Sources
- REBELS-IFU: on the origin of the elevated [OIII]/[CII] ratios in the early Universe
- Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7
- ALMA Observations of [OI]145um and [NII]205um Emission lines from Star-Forming Galaxies at $z\sim7$
- ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at $z\simeq1-8$
- Evidence for inefficient dust production in a massive, metal-rich galaxy at z=7.13 uncovered by JWST and ALMA
- GA-NIFS: interstellar medium properties and tidal interactions in the evolved massive merging system B14-65666 at z=7.152
- UNCOVER/MegaScience Finds Uniform and Highly Bursty Star Formation at 3 < z < 9, consistent with the High-Redshift UV Luminosity Function
- Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation
- The Drivers of Cosmic Dust Temperature Evolution
- Fine-structure Line Atlas for Multi-wavelength Extragalactic Study (FLAMES) III: [C II] as Tracer, Crisis of SFR, [O III]/[C II] at High-z, New Answers and New Questions
- Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15
- REBELS-IFU: Evidence for metal-rich massive galaxies at z~6-8
- The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10
- DREAMS. JWST Spectroscopy of a $z=8.3$ Galaxy with an ALMA Dust Continuum Detection: Early Dust, Very High $T_{\rm dust}$, and a Multi-wavelength [OIII] Ratio Discrepancy
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