Table 1: A sample of results from the automatic analyses. We list the names, HD numbers and spectral types from the manual spectral typing. We give the $T_{\rm eff}$ , $\log g$ and [Fe/H] and estimated uncertainties determined by VASP and VWA. $v \sin i$ values are calculated with VWA and have uncertainties of 10-20%. The first four targets are not VSOP targets, but high S/N HARPS spectra taken from Dall et al. (2006), which we have used to calibrate our tools. Full detailed results for all VSOP stars can be found online (see text).
Star Spectral $v \sin i$ VASP VWA

HD type [km s^-1] $T_{\rm eff}$ [K] $\log g$ [Fe/H] $T_{\rm eff}$ [K] $\log g$ [Fe/H]

$\alpha$ Hor 26967 K1III 2 4675(143) 2.8(4) +0.22(13) 4550(80) 2.2(2) -0.02(5)

$\tau$ Cet 10700 G8V 3 5292(157) 4.6(4) -0.45(15) 5320(50) 4.5(1) -0.47(5)

Sun - G2V 2 5842(168) 4.5(4) -0.16(16) 5810(40) 4.5(1) -0.07(3)

$\gamma$ Ser 142860 F6IV 11 6322(191) 4.1(7) -0.18(20) 6250(80) 4.1(1) -0.24(5)

ZZ Pyx - K3V 5 4228(223) 1.4(1) -0.31(13) 3900(150) 1.4(3) -1.3(2)

V349 Vel 91021 F2+? 16 7314(241) 5.2(9) -0.89(54) 7200(150) 4.0(2) -0.43(5)

LP Vir 115466 F1IV 40 7031(194) 3.4(8) -0.32(29) 7030(80) 3.7(1) -0.13(5)

V976 Cen 118551 F0III 40 7048(203) 2.0(7) -0.16(23) 8400(100) 2.4(2) -0.78(5)

PP Hya 87130 A5V 80 7924(219) 4.0(8) -1.35(73) - - -

**Table 1:** A sample of results from the automatic analyses. We list the names, HD numbers and spectral types from the manual spectral typing. We give the $T_{\rm eff}$ , $\log g$ and [Fe/H] and estimated uncertainties determined by VASP and VWA. $v \sin i$ values are calculated with VWA and have uncertainties of 10-20%. The first four targets are not VSOP targets, but high S/N HARPS spectra taken from Dall et al. (2006), which we have used to calibrate our tools. Full detailed results for all VSOP stars can be found online (see text).
Star		Spectral	$v \sin i$	VASP	VWA
	HD	type	[km s^-1]	$T_{\rm eff}$ [K]	$\log g$	[Fe/H]	$T_{\rm eff}$ [K]	$\log g$	[Fe/H]
$\alpha$ Hor	26967	K1III	2	4675(143)	2.8(4)	+0.22(13)	4550(80)	2.2(2)	-0.02(5)
$\tau$ Cet	10700	G8V	3	5292(157)	4.6(4)	-0.45(15)	5320(50)	4.5(1)	-0.47(5)
Sun	-	G2V	2	5842(168)	4.5(4)	-0.16(16)	5810(40)	4.5(1)	-0.07(3)
$\gamma$ Ser	142860	F6IV	11	6322(191)	4.1(7)	-0.18(20)	6250(80)	4.1(1)	-0.24(5)
ZZ Pyx	-	K3V	5	4228(223)	1.4(1)	-0.31(13)	3900(150)	1.4(3)	-1.3(2)
V349 Vel	91021	F2+?	16	7314(241)	5.2(9)	-0.89(54)	7200(150)	4.0(2)	-0.43(5)
LP Vir	115466	F1IV	40	7031(194)	3.4(8)	-0.32(29)	7030(80)	3.7(1)	-0.13(5)
V976 Cen	118551	F0III	40	7048(203)	2.0(7)	-0.16(23)	8400(100)	2.4(2)	-0.78(5)
PP Hya	87130	A5V	80	7924(219)	4.0(8)	-1.35(73)	-	-	-

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