A Hubble-like sequence of galaxy morphologies exists by redshift 4, with low-mass galaxies as persistent star-forming disks and massive galaxies following either stable disk or rapid compaction-quenching paths.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Morphological metrics in galaxy images suffer systematic biases from resolution, depth, and noise that can be quantified and corrected empirically, with new metrics proposed to reduce those effects.
New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.
citing papers explorer
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The Hubble sequence in JWST CEERS from unbiased galaxy morphologies
A Hubble-like sequence of galaxy morphologies exists by redshift 4, with low-mass galaxies as persistent star-forming disks and massive galaxies following either stable disk or rapid compaction-quenching paths.
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statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys
Morphological metrics in galaxy images suffer systematic biases from resolution, depth, and noise that can be quantified and corrected empirically, with new metrics proposed to reduce those effects.
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The integral and correlation scales of solar wind turbulence
New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.