Calibration of Strömgren uvby-Hβ photometry for late-type stars – a model atmosphere approach

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Table 1:

Standard deviations for $T_{\rm eff}$ and [Fe/H] derived using models as compared with literature values of the different comparison samples. See also Figs. 7-9 and Figs. 13, 14.
		$T_{\rm eff}$		[Fe/H]
	Dwarfs		Giants	G-stars	F-stars
Theoretical	(b-y)	H $\beta$	(b-y)
Standard	133	151	144	0.263	0.254
C06	101	-	-	0.321	0.190
VF05	185	-	-	0.392	0.399
All	172	-	-	0.368	0.355
A06,99 + S&N89	A06		A99	S&N89
Standard	110	156	116	0.183	0.182
C06	118	-	-	0.158	0.128
VF05	135	-	-	0.128	0.146
All	130	-	-	0.141	0.157
HNA07
Standard	101	-	-	0.209	0.164
C06	92	-	-	0.159	0.132
VF05	101	-	-	0.123	0.130
All	100	-	-	0.144	0.140
RM05
Standard	155	-	105	0.268	0.176
C06	110	-	-	0.176	0.139
VF05	128	-	-	0.116	0.081
All	134	-	-	0.161	0.122

Source LaTeX | All tables | In the text

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