Open Access

Table 3

Isochrone models currently supported by madys with their bibliographic references.

Name Y0 Z M m t Myr c.p. Reference
ATMO2020 0.275 0.0169 [0.001, 0.075] [100,104] Phillips et al. (2020)
B97 0.27431 0.01886 [10−3,0.04] [100,104] Burrows et al. (1997)
BEX 0.27 0.0142 [1.5 × 10−5,0.002] [1,4 × 103] Linder et al. (2019); Marleau et al. (2019)
BHAC15 0.271 0.0153 [0.01,1.4] [0.5, 104] Baraffe et al. (2015)
Geneva 0.266 0.014 [0.8,120] [0.1, 102] Haemmerlé et al. (2019)
MIST 0.2703 0.0142 [0.1,150] [10−1, 2 × 104] m, α, v Dotter (2016); Choi et al. (2016)
PARSEC 0.2485 0.01524 [0.09,350] [10−1,104] m Marigo et al. (2017)
(PHOENIX) AMES-COND 0.247 0.018 [0.005,1.4] [1,1.2 × 104] Allard et al. (2001)
(PHOENIX) AMES-Dusty 0.247 0.018 [0.005,1.4] [1,1.2 × 104] Allard et al. (2001)
(PHOENIX) Bt-Settl 0.271 0.0153 [0.01,1.4] [100,104] Allard (2016)
(PHOENIX) NextGen 0.247 0.018 [0.01,1.4] [100,1.2 × 104] Hauschildt et al. (1999)
PM13 - - [0.075,27] Pecaut & Mamajek (2013)
SB12 0.27431 0.01886 [10−3,10−2] [1,100] Spiegel & Burrows (2012)
Sonora Bobcat 0.2735 0.0153 [5 × 10−4,10−1] [10−1,104] Marley et al. (2021)
SPOTS 0.2676 0.0165 [0.1,1.3] [100,4 × 103] s Somers et al. (2020)
STAREVOL 0.269 0.0134 [0.2,1.5] [1,1.26 × 104] m, v Amard et al. (2019)
YAPSI 0.2775 0.0142 [0.15,5] [0.5,104] m, Y Spada et al. (2017)

Notes. Adopted values for solar metallicity (Z) and the initial helium abundance (Y0) are reported (u = unknown), together with mass (M) and age ranges (t). Customizable parameters (c.p.): metallicity (m), helium content (Y), alpha enhancement (α), rotational velocity (v), spot fraction (s).

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