We present the Str\u00f6mgren photometry for star clusters and their surrounding fields in the Large Magellanic Cloud (LMC) for which all three Str\u00f6mgren vby filters were available and subsequently color indices (b-y) and m1 could be calculated. Data were collected with 4.1-m SOAR telescope located in Cerro Pach\u00f3n, Chile, and equipped with the SOI camera with field of view of 5.26\u2019x5.26\u2032 and pixel scale of 0.154\u2033\/pix during two runs: December 17-19, 2008 and January 16-18, 2009.<\/p>\n\n\n\n
Photometric errors are presented in two columns, depending on the method used for their evaluation: i) the DAOPHOT package or ii) full error propagation of the transformation equations.<\/p>\n\n\n\n
Presented photometry is a complete version of Table 2 from a paper Metallicities and ages for star clusters and their surrounding fields in the Large Magellanic Cloud<\/em> (Narloch et al. 2022, A&A 666, A80<\/a>)<\/p>\n\n\n\n