Authors: Salih KARAALİ
Abstract: Comparison of metallicities for stars in SA141 and SA57 determined by means of four methods, i,e.: Buser and Fenkart: photographically, Cayrel et al: synthetic spectra, Pel et al: Walraven photometry, and Croswell et al: Str\"{o}mgren photometry are presented. Large scattering and systematic deviation in Figure 1 and Figure 2 indicate that metallicities with [Fe/H] Keywords: Photometry-stars: abundances-Basel Field SA141- Basel Field SA57
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