The average dust attenuation law at 2<z<7 is empirically measured from stacked SEDs and matches the local starburst curve with R_V=3.98, a flatter UV slope, and no 2175A bump.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Extended [CII] emission reveals a large cold gas halo around the z=7.27 quiescent galaxy RUBIES-UDS-QG-z7, with gas mass estimates indicating f_gas >20% and possible past AGN-driven outflow.
JWST prism spectroscopy of 200 massive galaxies at z~3-15 shows normal star-forming galaxies dominate at z>6 while dusty systems and quiescent galaxies increase at lower redshift, with evidence for multiple quenching pathways.
citing papers explorer
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A first empirical derivation of the average dust attenuation law at 2<z<7
The average dust attenuation law at 2<z<7 is empirically measured from stacked SEDs and matches the local starburst curve with R_V=3.98, a flatter UV slope, and no 2175A bump.
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Extended [CII] gas emission in and around a massive quiescent galaxy at z=7.3
Extended [CII] emission reveals a large cold gas halo around the z=7.27 quiescent galaxy RUBIES-UDS-QG-z7, with gas mass estimates indicating f_gas >20% and possible past AGN-driven outflow.
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A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec $\sim$3-15
JWST prism spectroscopy of 200 massive galaxies at z~3-15 shows normal star-forming galaxies dominate at z>6 while dusty systems and quiescent galaxies increase at lower redshift, with evidence for multiple quenching pathways.