MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
The paper outlines the science case and current development status of the Maunakea Spectroscopic Explorer as a next-generation facility for spectroscopic surveys.
citing papers explorer
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Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
MESA Star has been substantially updated with new capabilities for low-mass giant planets, asteroseismology coupling, rotating star models, and uninterrupted massive star evolution to core collapse.
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Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman
IllustrisTNG simulations link filament density to galaxy morphology trends across redshifts and predict that Roman's planned HLWAS survey needs greater depth to accurately map the z=1 cosmic web.
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The Maunakea Spectroscopic Explorer
The paper outlines the science case and current development status of the Maunakea Spectroscopic Explorer as a next-generation facility for spectroscopic surveys.