5 citations · 9 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2026
Chromospheric sensitivity of stellar spectral lines: an unsupervised machine learning classification
Juan I. Peralta, Mariela C. Vieytes
Stellar magnetic activity alters thousands of spectral lines, limiting high-precision radial-velocity measurements, abundance analyses, and planetary characterization. We present a…
astro-ph.SR2023★ 5 cited
Modeling the Mg I from the NUV to MIR. II. Testing stellar models
J. I. Peralta, M. C. Vieytes, A. M. P. Mendez +1
Aims. We tested the new atomic model using atmospheric models of stars of different spectral types: the Sun (dG2), HD22049 (dK2, Epsilon Eridani), GJ 832 (dM2), and GJ 581 (dM3). M…
astro-ph.SR2021★ 4 cited
Modeling the MgI from the NUV to MIR: I. The Solar Case
J. I. Peralta, M. C. Vieytes, A. M. P. Mendez +1
Semi-empirical models of the solar atmosphere are used to study the radiative environment of any planet in our solar system. There is a need for reliable atomic data for neutral at…