Parses Pipeline For Determining The Stellar Parameters

PARSES is a pipeline for determining physical parameters of a star from the stellar spectra -- effective temperature, metallicity, surface gravity and rotational velocity. It utilizes the grid of templates based on synthetic spectra, and the search routine is based on the Minimum Distance Method. In order to calibrate the routine, we tested it with different wavelength ranges used for fitting the observed spectra. Results for stellar parameters are compared with the literature values from the ELODIE library. The last step was to choose final solution for full implementation on the data produced with the STELLA telescope. The modified version of the pipeline is going to be used in processing the data from the ELODIE spectral library and also tested on some Gaia ESO data.