All Tables
- Table 1:
Comparison of the principal characteristics of publically
available libraries of synthetic spectra with resolution
better than 5 Å. N: number of combinations of
atmospheric parameters and rotational velocities. new
ODF: use of the new opacity distribution functions.
TiO: inclusion of the TiO line-list. pred. lines:
inclusion of the "predicted lines''. The last three columns
indicate if the spectra are provided for different values of
enhancement of
-elements, micro-turbulence velocity
and rotational velocity.
- Table 2:
Range of atmospheric parameters explored by our synthetic spectral library.
- Table 3:
Naming scheme for the spectra contained in the library.
- Table 4:
Comparison between different calibrations for colors and temperatures
of late type main sequence stars.
a: Bessell (1990);
b: Bessell (1995);
c: Straizys (1992);
d: Bertone et al. (2004) using Kurucz spectra;
e: Bertone et al. (2004) using Phoenix spectra;
f: Drilling & Landolt (2000);
g: Straizys & Kuriliene (1981).