no code implementations • 21 Jan 2021 • V. Ripepi, G. Catanzaro, L. Molńar, E. Plachy, M. Marconi, G. Clementini, R. Molinaro, G. De Somma, S. Leccia, S. Mancino, I. Musella, F. Cusano, V. Testa
We have used high-resolution spectra obtained with HARPS-N@TNG for HD 344787 and the more famous Polaris DCEP, to infer their detailed chemical abundances.
Time Series Analysis Solar and Stellar Astrophysics