9 Additional Tables


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 Teff, K ΔV ff,% Tspot, K ΔT,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]
λ 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]
σ 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 6: Magnetic field measurement results.
Star Sp. class B, kG f, % Reference
G–K dwarfs and subgiants
HII 1100 K3V 2.50 ± 0.09 50 Valenti and Johns-Krull (2001Jump To The Next Citation Point)
𝜖 Eri K2V 1.44 ± 0.15 9 Valenti et al. (1995)
ξ Boo B K4V 2.3 20 Saar (1994Jump To The Next Citation Point)
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 (1994Jump To The Next Citation Point)
3.0 70 Valenti and Johns-Krull (2001Jump To The Next Citation Point)
AU Mic M1.6Ve 4.2 55 Saar (1994Jump To The Next Citation Point)
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 (1996Jump To The Next Citation Point)
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)


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