ASCL Code Record
[ascl:2111.016]
SteParSyn: Stellar atmospheric parameters using the spectral synthesis method
SteParSyn infers stellar atmospheric parameters (Teff, log g, [Fe/H], and Vbroad) of FGKM-type stars using the spectral synthesis method. The code uses the MCMC sampler emcee (ascl:1303.002) in conjunction with an spectral emulator that can interpolate spectra down to a precision < 1%. A grid of synthetic spectra that allow the user to characterize the spectra of FGKM-type stars with parameters in the range of 3500 to 7000 K in Teff, 0.0 to 5.5 dex in log g, and −2.0 to 1.0 dex in [Fe/H] is also provided.
- Code site:
- https://github.com/hmtabernero/SteParSyn
- Described in:
- https://ui.adsabs.harvard.edu/abs/2022A%26A...657A..66T
- Bibcode:
- 2021ascl.soft11016T
Preferred citation method:
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