Automated Analysis of STELLA Spectra
Some 10 years ago we developed a code, PARSES, to extract stellar
atmospheric
parameters from high-resolution STELLA spectra. In the mean time much
progress
has taken place in the field of automated spectroscopic pipeline, fueled
by a long
list of past, ongoing and future surveys. I will take this opportunity
to recap lessons
learned, and discuss the way forward to upgrade PARSES and maximize the
future
exploitation of STELLA and its niche in the current scientific landscape.