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[ascl:1402.016] FAMA: Fast Automatic MOOG Analysis

FAMA (Fast Automatic MOOG Analysis), written in Perl, computes the atmospheric parameters and abundances of a large number of stars using measurements of equivalent widths (EWs) automatically and independently of any subjective approach. Based on the widely-used MOOG code, it simultaneously searches for three equilibria, excitation equilibrium, ionization balance, and the relationship between logn(FeI) and the reduced EWs. FAMA also evaluates the statistical errors on individual element abundances and errors due to the uncertainties in the stellar parameters. Convergence criteria are not fixed "a priori" but instead are based on the quality of the spectra.

Code site:
http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/558/A38
Described in:
https://ui.adsabs.harvard.edu/abs/2013A%26A...558A..38M
Bibcode:
2014ascl.soft02016M

Views: 4830

ascl:1402.016
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