Table B.1: The temperature conversion scales for dwarfs at spectral types G0-M 9. For details on the references see Table 2. Temperatures are given in [K].
Spectral type bessell79911 ck792 djn873 hss944 kh955 luhman036 tokunaga007
G0 6000 5900 5940 6026 6030   5930
G1   5830     5945    
G2   5770 5790 5860 5860   5830
G3         5830    
G4     5640   5800   5740
G5   5660   5754 5770    
G6 5500       5700   5620
G7         5630    
G8   5450 5310 5572 5520    
G9         5410    
K0   5240 5150 5248 5250   5240
K1   5110 4990 5082 5080    
K2 5000 4950   4898 4900   5010
K3   4780 4690 4732 4730    
K4 4500 4580 4540 4592 4590   4560
K5   4400 4410 4395 4350   4340
K6   4200     4205    
K7 4000 4000 4150 3999 4060   4040
K7-M0   3960          
K9     3940        
M0 3800 3920 3840 3802 3850   3800
M0.5   3800   3724      
M 1 3650 3680 3660 3648 3720 3680 3680
M 1.5   3590 3590 3573      
M 2 3500 3500 3520 3499 3580 3510 3530
M 2.5   3430          
M 3 3350 3360 3400 3350 3470 3350 3380
M 3.5   3300          
M 4 3150 3230 3290 3148 3370 3180 3180
M 4.5              
M 5 3000 3120 3170 2999 3240 2960 3030
M 5.5 2900 3040          
M 6 2800 2960 3030 2799 3050 2740 2850
M 6.5 2700   2950        
M 7 2600   2860     2620  
M 7.5 2450            
M 8     2670     2500  
M 9     2440     2300  
1 bessell7991 = combination of Bessell (1979) and Bessell (1991); 2 ck79 = Cohen & Kuhi (1979); 3 djn87 = de Jager & Nieuwenhuijzen (1987); 4 hss94 = Hartigan et al. (1994); 5 kh95 = Kenyon & Hartmann (1995); 6 luhman03 = Luhman et al. (2003); 7 tokunaga00 = Tokunaga (2000).

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Article Contents
1 Introduction
2 A new method - extending the approach of White et al. (1999)
3 Application to known eclipsing binaries
4 Summary and conclusions
References
Online Material
Appendix A: Derivation of intrinsic scale errors
Appendix B: Conversion tables
List of tables
List of figures