activity
20122020
most citedODUSSEAS: A machine learning tool to derive effective temperature and metallicity for M dwarf stars

50 citations · 193 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2020★ 50 cited

ODUSSEAS: A machine learning tool to derive effective temperature and metallicity for M dwarf stars

A. Antoniadis-Karnavas, S. G. Sousa, E. Delgado-Mena +3

Aims. The derivation of spectroscopic parameters for M dwarf stars is very important in the fields of stellar and exoplanet characterization. The goal of this work is the creation…

astro-ph.SR2018★ 2 cited

Exploring the stellar properties of M dwarfs with high-resolution spectroscopy from the optical to the near-infrared

A. S. Rajpurohit, F. Allard, S. Rajpurohit +4

Context. Being the most numerous and oldest stars in the galaxy, M dwarfs are objects of great interest for exoplanet searches. The presence of molecules in their atmosphere compli…

astro-ph.SR2018★ 15 cited

Photometric variability of massive young stellar objects. I

G. D. C. Teixeira, M. S. N. Kumar, L. Smith +8

The VVV survey has allowed for an unprecedented number of multi-epoch observations of the southern Galactic plane. In a recent paper,13 massive young stellar objects(MYSOs) have al…

astro-ph.SR2017★ 26 cited

Atmospheric stellar parameters for large surveys using FASMA, a new spectral synthesis package

M. Tsantaki, D. T. Andreasen, G. D. C. Teixeira +4

In the era of vast spectroscopic surveys focusing on Galactic stellar populations, astronomers want to exploit the large quantity and good quality of data to derive their atmospher…

astro-ph.SR2017★ 31 cited

Photospheric properties and fundamental parameters of M dwarfs

A. S. Rajpurohit, F. Allard, G. D. C. Teixeira +3

M dwarfs are an important source of information when studying and probing the lower end of the Hertzsprung-Russell (HR) diagram, down to the hydrogen-burning limit. Being the most…

astro-ph.SR2017★ 41 cited

SWEET-Cat update and FASMA. A new minimization procedure for stellar parameters using high-quality spectra

D. T. Andreasen, S. G. Sousa, M. Tsantaki +6

Context: Thanks to the importance that the star-planet relation has to our understanding of the planet formation process, the precise determination of stellar parameters for the ev…