Combining dating methods for better stellar ages
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Updated
Sep 18, 2019 - Jupyter Notebook
Combining dating methods for better stellar ages
Friendly user interface to estimate vsini, using high resolution spectra, based on Fourier's method.
A comparison of covariance functions used to infer stellar rotation periods of stars
Reproducible code and derived data for testing how present-day stellar constraints identify cumulative EUV and wind histories in TOI-700 and LHS 1140.
ML classification of stellar variability in the Praesepe (M44) open cluster using Gaia DR3 and TESS.
Core GCNS, Gaia DR3, and TESS periodic-variability analysis pipeline
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