Table 5
Description of hounds in group 1 (forward modelling).
| Method | Participant(s) | Optimisation procedure | Evol. code | Constraints | References |
|
|
|||||
| GOE | WHB | Grid search + Nelder-Mead | MESA | freq. | Appourchaux et al. (2015) |
| YMCM | SB | Monte Carlo analysis | YREC | freq., & ratios | Silva Aguirre et al. (2015) |
| ASTFIT | JCD | Scan evolutionary sequences | ASTEC | freq. | Silva Aguirre et al. (2015) |
| YL | YL | Levenberg-Marquardt | CESAM2k | freq. | Lebreton & Goupil (2014) |
| AMP | TM | Genetic algorithm | ASTEC | freq., & ratios | Metcalfe et al. (2009, 2014) |
| BASTA | VSA | Bayesian grid scan | GARSTEC | ratios | Silva Aguirre et al. (2015) |
| MESAastero | DS | Grid search + Nelder-Mead | MESA | freq. | Paxton et al. (2013, 2015) |
| V&A, grid | KV & HMA | Scan evolutionary sequences | MESA | freq. | Verma et al. (2014b) |
Notes. YMCM = Yale-Monte Carlo Method; ASTFIT = ASTEC Fitting method; AMP = Asteroseismic Modeling Portal; BASTA = BAyesian STellar Algorithm; YREC = Yale Rotating stellar Evolution Code (Demarque et al. 2008); ASTEC = Aarhus STellar Evolution Code (Christensen-Dalsgaard 2008b); CESAM = Code d’Evolution Stellaire Adaptatif et Modulaire (Morel & Lebreton 2008); MESA = Modules for Experiments in Stellar Astrophysics (Paxton et al. 2011, 2013, 2015); GARSTEC = GARching STellar Evolution Code (Weiss & Schlattl 2008).
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