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A program for automatic two-dimensional quantification of stars observed in the Vilnius photometric system (i.e., determination of the spectral type and absolute magnitude My) has been proposed by Jasevicius (1986). However, this program takes a lot of time to determine the parameters for each star and is, therefore, not a particularly convenient tool when a huge amount of data (say, from CCD photometry) is involved. We have made an attempt to develop a more comfortable and prompt program for this purpose.

A computer program for two-dimensional quantification of normal stars in the Vilnius photometric system