no code implementations • 11 Jan 2021 • N. Casasayas-Barris, E. Palle, M. Stangret, V Bourrier, H. M. Tabernero, F. Yan, F. Borsa, R. Allart, M. R. Zapatero Osorio, C. Lovis, S. G. Sousa, G. Chen, M. Oshagh, N. C. Santos, F. Pepe, R. Rebolo, P. Molaro, S. Cristiani, V. Adibekyan, Y. Alibert, C. Allende Prieto, F. Bouchy, O. D. S. Demangeon, P. Di Marcantonio, V. D Odorico, D. Ehrenreich, P. Figueira, R. Génova Santos, J. I. González Hernández, B. Lavie, J. Lillo-Box, G. Lo Curto, C. J. A. P. Martins, A. Mehner, G. Micela, N. J. Nunes, E. Poretti, A. Sozzetti, A. Suárez Mascareño, S. Udry
We observed two transits of the iconic gas giant HD 209458b between 380 and 780 nm, using the high-resolution ESPRESSO spectrograph.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
no code implementations • 18 Nov 2020 • H. M. Tabernero, R. Dorda, I. Negueruela, E. Marfil
Secondly, unlike any known RSG or RHG, VX Sgr displays strong Rb I lines.
Solar and Stellar Astrophysics
1 code implementation • 15 Jul 2019 • H. M. Tabernero, E. Marfil, D. Montes, J. I. González Hernández
Context: StePar is an automatic code written in Python 3. X designed to compute the stellar atmospheric parameters Teff, log(g), [Fe/H], and of FGK-type stars by means of the EW method.
Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics
