Table 3: Stellar parameters used to for the calculation of (1.) the M ARCS model atmosphere spectra (Cols. 2-5) and (2.) the Engelke function and blackbody (BB) (Cols. 6, 7) in Fig. 10. Effective temperature, T, is given in Kelvin, gravity, g, in cm/s², and angular diameter, $\theta_{\rm d}^{}$ , in mas.
Engelke and BB

target T_eff log g [Fe/H] $\theta_{\rm d}^{}$ T_eff $\theta_{\rm d}^{}$

$\xi$ Dra 4440 2.40 0.10 3.09 4440 3.09

$\alpha$ Boo 4320 1.50 -0.50 20.66 4362 21.12

$\alpha$ Tuc 4300 1.35 0.00 5.90 4300 5.90

$\beta$ And 3880 0.95 0.00 13.48 3839 13.71

**Table 3:** Stellar parameters used to for the calculation of *(1.)* the M ARCS model atmosphere spectra (Cols. 2-5) and *(2.)* the Engelke function and blackbody (BB) (Cols. 6, 7) in Fig. 10. Effective temperature, T, is given in Kelvin, gravity, g, in cm/s², and angular diameter, $\theta_{\rm d}^{}$ , in mas.
		Engelke and BB
target	T_eff	log g	[Fe/H]	$\theta_{\rm d}^{}$	T_eff	$\theta_{\rm d}^{}$
$\xi$ Dra	4440	2.40	0.10	3.09	4440	3.09
$\alpha$ Boo	4320	1.50	-0.50	20.66	4362	21.12
$\alpha$ Tuc	4300	1.35	0.00	5.90	4300	5.90
$\beta$ And	3880	0.95	0.00	13.48	3839	13.71

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