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Table D.1.

Templates included in eazy-py to account for stellar contaminants.

Name Reference Type Number log g [cm s2] Teff [K] [M/H] Coverage [μm]
(1) (2) (3) (4) (5) (6) (7) (8)
Sonora 2018 Marley et al. (2018) Theoretical 420 [3.25, 5.5] [200, 2400] 0 [0.4, 40]
Lowz Library Meisner et al. (2021) Theoretical 374a 3.5, 5 [500, 1600] [-2.5, 1] [0.1, 10]

AMES-Dusty Allard et al. (2001) Theoretical 16 4.5 [500, 2000] 0 [0.1, 10]
Baraffe et al. (2003)
Grevesse et al. (1993)
Partridge & Schwenke (1997)

AMES-Cond Allard et al. (2001) Theoretical 11 4.5 [800,1900] 0 [0.1, 10]
Chabrier et al. (2000)
Grevesse et al. (1993)
Partridge & Schwenke (1997)

NextGen Allard et al. (1997) Theoretical 8 4.5 [2200, 9800] 0 [0.01, 921]
Baraffe et al. (1997, 1998)
Grevesse et al. (1993)
Hauschildt et al. (1999)
Schryber et al. (1995)

SpeX Prism Libraryb Burgasser et al. (2006) Empirical 149 [0.6, 2.5]
Burgasser (2014)

L and T dwarf data archive c Knapp et al. (2004) Empirical 148 [0.1, 2.5]
Chiu et al. (2006)
Golimowski et al. (2004)

TRDS Pickles Atlasd Pickles (1998) Empirical 131 [2951.21, 39810.7] [0.115, 2.5]

a This subsample is defined by a carbon-to-oxygen ratio C/O = 0.55 and vertical eddy diffusion coefficient log10Kzz = 2.0. b These templates were extended to 0.1 μm and 100 μm by assuming Wien and Rayleigh-Jeans emission tails, respectively. c Find compilation at http://svo2.cab.inta-csic.es/theory/newov2/index.php?. d TRDS Pickles Atlas account for all normal spectral types and luminosity classes at solar abundance, as well as metal-weak and metal-rich F-K dwarf and G-K giant stars. Notes: Col (1): Template set name; Col (2): references; Col (3): type templates: either from a theoretical grid or empirical observed spectra; Col (4): number of templates included; Col (5): logarithm of the surface gravity; Col (6): Effective temperature; Col (7): logarithm of the ratio of the mass fraction of metals to the mass fraction of hydrogen, compared to the solar value; Col (8): lower and upper limits of the wavelength coverage.

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