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Table 2:

Quantities for the same GCs, derived by our works.

NGC
$\log T_{\rm eff}^{\rm max}$ IQR[Na/O] 1 P2 I2 E2 $\langle [\alpha/{\rm Fe}] \rangle$3 [(Mg+Al+Si) [Mg/Fe]$_{\max}^6$ [Mg/Fe]$_{\min}^6$ [Si/Fe] $_{\rm min}^6$ [Si/Fe] $_{\rm max}^6$
  (HB)           /Fe]6        

104
3.7564 0.472 27 69 4 0.42 0.46 0.60 +0.47 0.35 0.43
288 4.2215 0.776 33 61 6 0.42 0.41 0.55 +0.41 0.30 0.41
1904 4.3524 0.759 40 50 10 0.31 0.31 0.40 +0.16 0.25 0.34
2808 4.5684 0.999 50 32 18 0.33 0.29 0.42 -0.30 0.22 0.38
3201 4.0794 0.634 35 56 9 0.33 0.32 0.45 +0.27 0.25 0.41
4590 4.0414 0.372 40 60 0 0.35 0.40 0.48 +0.28 0.30 0.48
5904 4.1764 0.741 27 66 7 0.38 0.36 0.55 +0.31 0.21 0.39
6121 3.9685 0.373 30 70 0 0.51 0.54 0.65 +0.50 0.45 0.64
6171 3.8754 0.522 33 60 7 0.49 0.53 0.60 +0.46 0.45 0.63
6218 4.2174 0.863 24 73 3 0.41 0.43 0.60 +0.46 0.22 0.43
6254 4.4005 0.565 38 60 2 0.37 0.37 0.58 +0.33 0.18 0.36
6388 4.2554 0.795 41 41 19 0.22 0.30 0.40 +0.16 0.20 0.46
6397 3.9784 0.274 25 75 0 0.36   0.55 +0.40 0.25 0.43
6441 4.2304 0.660 38 48 14 0.21 0.34 0.45 +0.20 0.15 0.45
6752 4.4715 0.772 27 71 2 0.43 0.44 0.60 +0.36 0.28 0.49
6809 4.1535 0.725 20 77 2 0.42 0.43 0.60 +0.18 0.30 0.51
6838 3.7634 0.257 28 72 0 0.40 0.44 0.60 +0.39 0.30 0.51
7078 4.4774 0.501 39 61 0 0.40 0.46 0.68 -0.01 0.28 0.60
7099 4.0794 0.607 41 55 3 0.37 0.44 0.60 +0.44 0.20 0.45

Notes.  (1) IQR([Na/O]) comprises stars with GIRAFFE and UVES data; (2) P,I,E are fraction of stars of Primordial, Intermediate, Extreme populations from Paper VII; (3) [$\alpha $/Fe] is the average of [Mg/Fe] $_{\rm max}$, [Si/Fe] $_{\rm min}$and [Ca/Fe]; (4)  $\log T_{\rm eff}^{\rm max}$(HB) taken from Recio-Blanco et al. (2006); (5)  $\log T_{\rm eff}^{\rm max}$(HB) derived in the present work (see Sect. 5.2); (6) from Paper VIII.


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