9 Additional Tables

9 Additional Tables


Star	Sp	T $eff$ ,K	$DV$	ff,%	T $spot$ ,K	$D$ T,K	Method	Ref.




Giants and subgiants

HD199178	G5 III	5350		29(d)	3800 $±$ 200	1550	MBM	[1]
EI Eri	G5 IV	5600		36(d)	3700 $±$ 150	1900	MBM	[1]
$c$ And	G8 III	4750		23(d)	3650 $±$ 150	1100	MBM	[1]
HK Lac	K0 III	4790	0.14		3840 $±$ 200	950 $±$ 200	LCM	[3]
		4765	0.37	34(d)	3788 $±$ 10	977	LDR	[4]
XX Tri	K0 III	4820	0.63	20(s)	3500	1300	DI	[5]
		4750		35(d)	3420 $±$ 120	1320	MBM	[20]
HU Vir	K0 IV	5000		44(d)	3440 $±$ 100	1560	MBM	[1]
UX Ari	K0 IV	5000		48(d)	3500	1500	MBM	[2]
AR Lac	K0 IV	4700	0.04		3500	1200	LCM	[6]
$s$ Gem	K1 III	4600		33(d)	3850 $±$ 100	750	MBM	[1]
DM UMa	K1 III	4600		35(d)	3570 $±$ 100	1030	MBM	[1]
		4500		42(d)	3450 $±$ 120	1010	MBM	[20]
SZ Psc	K1 IV	4700			3500 $±$ 400	1200 $±$ 400	LCM	[7]
HR1099	K1 IV	4700		40(d)	3500	1200	MBM	[2]
		4700	0.09		3500	1200	LCM	[6]
HR7275	K2 III	4600		27(d)	3500 $±$ 150	1100	MBM	[1]

II Peg	K2 IV	4600	0.42	37(h)	3400 $±$ 100	1200 $±$ 100	LCM	[3]
		4750	0.16	50(d)	3530 $±$ 100	1220	MBM	[1]
		4750	0.23	43(d)	3530 $±$ 100	1220	MBM	[1]
		4500	0.25		3300	1200	LCM	[6]
		4600	0.25	20(d)	3500	1100	DI	[8]
IM Peg	K2 III	4666	0.20	32(d)	3943 $±$ 10	723	LDR	[4]
		4450		20(d)	3450	1000	DI	[9]
IN Vir	K2 IV	4600		40(d)	3350 $±$ 170	1250	MBM	[20]
VY Ari	K3 IV	4916	0.41	41(d)	4007 $±$ 10	909	LDR	[4]
		4600	0.28	15(s)	3400	1200 $±$ 50	LCM	[10]
		4600	0.20	12(s)	3400	1200 $±$ 50	LCM	[10]
		4600	0.10	15(s)	3400	1200 $±$ 50	LCM	[10]



Dwarfs

Sun	G2 V	5870			4200(um)	1670
Sun	G2 V	5870			5000(pen)	870
HD307938	G2 V	5800	0.06	13(s)	3900	1900	DI+LC	[11]
EK Dra	G2 V	5930		6(s)	5400	500	LCM	[12]
		5850	0.08	11(d)	4800	1050	DI	[13]
		5830		40(d)	$>$ 3800	$<$ 2030	MBM	[20]
AB Dor	K0 V	5200	0.05	12(s)	4000	1200	LCM	[14]

		5200	0.12	5(s)	3700	1500	LCM	[14]
LQ Hya	K2 V	5175		45(d)	3650	1525	MBM	[2]
OU Gem	K3 V	4925		35(d)			MBM	[2]
V833 Tau	K4 V	4500		45(d)	3175	1325	MBM	[2]
EQ Vir	K5e	4380		45(d)	3350 $±$ 120	1030	MBM	[20]
BY Dra	M0 V	4100	0.08	34(h)	3500 $±$ 450	600 $±$ 450	LCM	[3]
		4100		60(d)	3700	400	LCM	[15]
		4100	0.10		3500	600	LCM	[6]
YY Gem	M0 V	3820			3400	400	LCM	[16]
AU Mic	M2e V	3500	0.10		2650	850	LCM	[6]
		3500	0.32	10(s)	3000	500	LCM	[17]
EV Lac	M4e V	3300	0.10	7(d)	3080	220	LCM	[18]



T Tauri stars

V410 Tau	K4	4300	0.38	32(d)	2900	1400	LCM	[19]
		4300	0.55	41(d)	2900	1400	LCM	[19]

Table 5:

A sample of starspot temperatures and filling factors. The filling factors are normalised to the stellar disk (d), hemisphere (h) or whole surface (s). For the stellar disk normalisation maximum observed filling factors are given. Different measurements for the same star from the same publication correspond to different seasons of observations. References: [1] O’Neal et al. (1998 ), [2] O’Neal et al. (2001 ), [3] Vogt (1981 ), [4] Catalano et al. (2002 ), [5] Strassmeier (1999 ), [6] Rodonò et al. (1986 ), [7] Eaton and Hall (1979 ), [8] Berdyugina et al. (1999a ), [9] Berdyugina et al. (2000 ), [10] Strassmeier and Bopp (1992 ), [11] Marsden et al. (2005 ), [12] Dorren and Guinan (1994 ), [13] Strassmeier and Rice (1998 ), [14] Amado et al. (2001 ), [15] Chugainov (1976 ), [16] Torres and Ribas (2002 ), [17] Torres and Ferraz Mello (1973 ), [18] Abranin et al. (1998 ), [19] Petrov et al. (1994 ), [20] O’Neal et al. (2004 ).


Star	Sp. class	B, kG	f, %	Reference





G-K dwarfs and subgiants

HII 1100	K3V	2.50 $±$ 0.09	50	Valenti and Johns-Krull (2001 )
$e$ Eri	K2V	1.44 $±$ 0.15	9	Valenti et al. (1995 )
$q$ Boo B	K4V	2.3	20	Saar (1994 )
VY Ari	K3IV	2.0 $±$ 0.3	66	Bopp et al. (1989 )





M dwarfs

AD Leo	M3.5Ve	3.80 $±$ 0.26	73	Saar and Linsky (1985 )
		4.0	65	Saar (1994 )
		3.0	70	Valenti and Johns-Krull (2001 )
AU Mic	M1.6Ve	4.2	55	Saar (1994 )
EQ Vir	K5Ve	2.5 $±$ 0.3	80	Saar et al. (1986 )
EV Lac	M4.5Ve	3.8 $±$ 0.5	50	Johns-Krull and Valenti (1996 )
		4.3	85	Saar (1994 )
GJ 729	M4.5Ve	2.6 $±$ 0.3	50	Johns-Krull and Valenti (1996 )
GJ 1049	M0V	5.0	50	Kochukhov et al. (2001 )





T Tau stars

BP Tau		2.46 $±$ 0.12		Johns-Krull et al. (1999a )
		2.6 $±$ 0.3		Johns-Krull et al. (1999b )
TW Hya		2.6	70	Valenti and Johns-Krull (2001 )

Table 6:

Magnetic field measurement results