Raw MPIA/1DNLTE Synthetic Spectra

This dataset comprises the raw high-resolution MPIA/1DNLTE synthetic spectra (using MAFAGS-OS model atmospheres), created with the online tool nlte.mpia.de/, for the purpose of predicting parameters for Gaia-ESO Survey FLAMES-UVES spectra. The NLTE corrections were made for H, O, Mg, Si, Ca, Ti, Cr, Mn, Fe, and Co. The wavelength range is 4830-5400A, and the parameter range is as follows:

• 4600K ≤ T_eff ≤ 8800K, step size 200K
• 1.0 ≤ logg ≤ 5.0, step size 0.2 dex
• -4.8 ≤ [Fe/H] ≤ 0.9, step size 0.3 dex
• -0.25 ≤ [α/Fe] ≤ 0.5, step size 0.25 dex (α elements considered: O, Ne, Mg, Si, S, Ar, Ca, and T)
• 1 km/s ≤ v_micro ≤ 2 km/s, step size 1 km/s