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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 ≤ Teff ≤ 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 ≤ vmicro ≤ 2 km/s, step size 1 km/s
stellar astrophysics, spectroscopy, spectra
stellar astrophysics, spectroscopy, spectra
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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