• Naming convention for the files:



	αMLT = 3.000	αMLT = 1.875	αMLT = 1.000	αMLT = 0.500
[Fe/H] = +0.3	X0p67336_Z0p03090_A3p000	X0p67336_Z0p03090_A1p875	X0p67336_Z0p03090_A1p000	X0p67336_Z0p03090_A0p500
[Fe/H] = 0.0	X0p70952_Z0p01631_A3p000	X0p70952_Z0p01631_A1p875	X0p70952_Z0p01631_A1p000	X0p70952_Z0p01631_A0p500
[Fe/H] = -0.5	X0p73671_Z0p00535_A3p000	X0p73671_Z0p00535_A1p875	X0p73671_Z0p00535_A1p000	X0p73671_Z0p00535_A0p500
[Fe/H] = -1.0	X0p74574_Z0p00171_A3p000	X0p74574_Z0p00171_A1p875	X0p74574_Z0p00171_A1p000	X0p74574_Z0p00171_A0p500
[Fe/H] = -1.5	X0p74865_Z0p00054_A3p000	X0p74865_Z0p00054_A1p875	X0p74865_Z0p00054_A1p000	X0p74865_Z0p00054_A0p500




• Content of the files:
• .track1 files:

Age	Xc	Yc	Zc	log L/L☉	log R/R☉	log g	log Teff	Ugrav	Xenv	Zenv	log Tc	η
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)

Columns: (1) age (Gyr); (2) hydrogen mass fraction in the center; (3) helium mass fraction in the center; (4) mass fraction of heavy elements in the center; (5) luminosity (L_☉ ); (6) radius (R_☉ ); (7) surface gravity (g cm^-2 ); (8) effective temperature (K); (9) fraction of energy produced by gravitational contraction (%); (10) hydrogen mass fraction at the surface; (11) mass fraction of heavy elements at the surface; (12) central temperature (K); (13) degeneracy parameter.


• .track2 files:

Age	Mcore/M*	Menvp/M*	Renvp/R*	τc	Icore	Ienvp	Itot
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)

Columns: (1) age (Gyr); (2) mass of the convective core (if present) (M_*); (3) mass of the convective envelope (M_*); (4) fractional radius at the bottom of the external convective envelope (R_*); (5) global convective turnover timescale (days); (6) moment of inertia of the convective core (if present) (g cm²); (7) moment of inertia of the external convective envelope (g cm²); (8) total moment of inertia of the star (g cm²).


• .iso1 files:

Mass	log Teff	log L/L☉	log g	MV	U-B	B-V	V-R	R-I
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)

Columns: (1) mass (M_☉); (2) effective temperature (K); (3) luminosity (L)_☉); (4) surface gravity (g cm^-2); (5) absolute V magnitude (mag); (6) U-B color index; (7) B-V color index; (8) V-R color index; (9) R-I color index.
Note: the Lejeune et al., 1998 T_eff-color transformation was used.


• .iso2 files:

Mass	log Teff	log L/L☉	log g	MV	U-B	B-V	V-R	R-I
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)

Columns: (1) mass (M_☉); (2) effective temperature (K); (3) luminosity (L)_☉); (4) surface gravity (g cm^-2); (5) absolute V magnitude (mag); (6) U-B color index; (7) B-V color index; (8) V-R color index; (9) R-I color index.
Note: the Van den Berg & Clem, 2003 T_eff-color transformation was used.





• Composition:
• (Z/X)_☉ = 0.0230, according to Grevesse & Sauval, 1998
• Enrichment law: Y = Y_p + ΔY/ΔZ, with Y = Y_p = 0.25 (primordial helium abundance), and ΔY/ΔZ = 1.48
• No α-elements enhancement: [α/H] = 0



• Surface atmospheric boundary conditions:
  PHOENIX BT-Settl atmospheric models (Allard et al., 2011)



• Mixing length parameter α_MLT (solar-calibrated):
  α_MLT = 1.875



• Other parameters:
• Diffusion of helium and heavy elements is included
• Core overshooting is ignored