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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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative 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.
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.
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.
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Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.