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).
\begin{table}
\par
\includegraphics[width=7.8cm,clip]{2490Tab4.ps}\end{table}

Source LaTeX | All tables | In the text