no code implementations • 16 Dec 2020 • A. Lançon, A. Gonneau, K. Verro, P. Prugniel, A. Arentsen, S. C. Trager, R. Peletier, Y. -P. Chen, P. Coelho, J. Falcón-Barroso, P. Hauschildt, T. -O. Husser, R. Jain, M. Lyubenova, L. Martins, P. Sánchez Blázquez, A. Vazdekis
When leaving the stellar parameters free to adjust, satisfactory representations of the SEDs are obtained down to about 4000 K. However, in particular below 5000 K and in the UVB spectral range, strong local residuals associated with intermediate resolution spectral features are then seen; the necessity of a compromise between reproducing the line spectra and reproducing the SEDs leads to dispersion between the parameters favored by various spectral ranges.
Solar and Stellar Astrophysics Astrophysics of Galaxies
