TY  - JOUR
AU  - Duque Arribas, Christian
AU  - Tabernero, H. M.
AU  - Montes Gutiérrez, David
AU  - Caballero, J. A.
AU  - Galceran, E.
PY  - 2025
DO  - 10.1051/0004-6361/202554722
SN  - 0004-6361
UR  - https://hdl.handle.net/20.500.14352/122890
T2  - Astronomy & Astrophysics
AB  - Context. M dwarfs are the most abundant stars in the Galaxy and serve as key targets for stellar and exoplanetary studies. It is particularly challenging to determine their metallicities because their spectra are complex. For this reason, several...
LA  - eng
M2  - L12-1
PB  - EDP Sciences
KW  - Stars: abundances
KW  - Stars: fundamental parameters
KW  - Hertzsprung–Russell and C–M diagrams
KW  - Stars: late-type
KW  - Stars: low-mass
TI  - A neural network approach to determining photometric metallicities of M-type dwarf stars
TY  - journal article
VL  - 698
ER  -