Semi-automated python wrapper for high-resolution optical spectroscopic analysis of evolved stars
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TO RUN A NEW STAR YOU NEED TO:
a) add the source's spectrum ("waveobs\tflux\terr\n") and the line regions ("wave_peak\twave_base\twave_top\tnote\n") to '.../mySample/input/' folder,
b) open the terminal in the root folder and type 'python Flug_opt.py 7-symbol-star-ID' (for example, "J005107").
a) images/ = iSpec logos (PNG and GIF),
b) input/ = iSpec input files: solar abundances, model atmospheres, model atmosphere grid and mini-grid (ATLAS, MARCS), line lists, and template spectra
c) isochrones/ = Yonsei-Yale isochrone plotter,
d) ispec/ = all PySpec essentials,
e) synthesizer/ = radiative transfer codes,
f) .git/ = iSpec git-related folder,
g) mySample/ = input and output files for E-iSpec,
h) dev-requirements.txt = Python requirements,
i) example.py = different examples of working with the PySpec functions,
j) Flug_linelist.py = a script to create atomic linelist,
k) Flug_opt.py = the main E-iSpec script,
l) interactive.py = GUISpec essential,
m) ispec.log = a concatenation of all the terminal logs (only iSpec-specific logs),
n) iSpec.command = a bash script invoking GUISpec,
o) LICENSE = iSpec license,
p) Makefile = subroutines initial builder (check iSpec installation manual),
q) pytest.ini = Python path testing,
r) README.md = iSpec readme,