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Table 3

Final results.

Feinstein 1 NGC 2168 NGC 2323 NGC 2437 NGC 2547

acorr = b + c(B − V)0,N 17(2)/55(6)/24 29(2)/47(17)/21 34(4)/35(17)/17 123(1)/61(6)/37 122(1)/82(6)/29
3σ ±8 ±9 ±14 ±12 ±9
N(>50%)/N(<50%) 22/6 19/8 9/9 36/12 16/17
#CP/Δa/Prob W16/+16/99 W244/+16/93 W171/+51/82 W172/+34/80 W8/+16/8
W17/+15/59 W336/+17/37 W457/+26/76
W364/+23/69 W469/+38/63
W476/+19/50
log Teff/log L/L 4.350/3.36 4.126/2.32 4.105/2.07 3.993/1.67 4.124/2.245
/ 4.060/2.25 4.018/1.82
4.086/2.77 3.978/1.98
3.985/1.72

NGC 4103 NGC 6025 NGC 6633 Stock 2 Trumpler 2

acorr = b + c(B − V)0,N 129(5)/151(25)/34 27(2)/101(16)/24 19(2)/70(11)/38 125(4)/118(21)/31 47(2)/60(14)/12
3σ ±14 ±13 ±14 ±15 ±20
N(>50%)/N(<50%) 21/13 23/5 28/12 24/10 9/5
#CP/Δa/Prob W48/+47/65 W6/+20/0 W30/+42/66
W77/24/4
log Teff/log L/L 3.919/0.92 3.988/1.49 4.069/2.12
/

Notes. All photometric values are given in mmag. For Feinstein 1 W17 and Stock 2 W77, we were not able to derive reliable astrophysical parameters (see text). The errors in the final digits of the corresponding quantity are given in parentheses.

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