At z=1, disk galaxies exhibit U-shaped stellar age profiles with turnover at the edge, indicating inside-out growth with approximately 300% mass increase in outer regions since z=0.
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2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
citing papers explorer
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Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST
At z=1, disk galaxies exhibit U-shaped stellar age profiles with turnover at the edge, indicating inside-out growth with approximately 300% mass increase in outer regions since z=0.
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The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.