Absolute dimensions of solar-type eclipsing binaries - EF Aquarii: a G0 test for stellar evolution models

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Table 9

The effective temperature determined with five different methods.

Method	Primary	Secondary

Alonso calibration^a	6128 ± 60	5205 ± 86
Holmberg calibration^b	6165 ± 68	5248 ± 109
Casagrande calibration^c	6244 ± 85	5301 ± 151
Popper flux scale^d	/	5098 ± 58
Spectroscopic temperature	6100 ± 50	5160 ± 103

References.

^(a)

Alonso et al. (1996),

^(b)

Holmberg et al. (2007),

^(c)

Casagrande et al. (2010),

^(d)

Popper (1980).

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