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Table 5.

Average offset and spread of adopted effective temperatures compared to the literature values, where ΔTeff = Teff, lit − Teff, SP_Ace/ATHOS.

Study Galaxy Method Tlit ⟨ΔTeffATHOS σTeff)ATHOS # ATHOS ⟨ΔTeffSP_Ace σTeff)SP_Ace # SP_Ace
Letarte et al. (2010) For Phot 261 1 −99 51 72
Kirby et al. (2010) For Fit/Spec −87 65 16
Kirby et al. (2013) For Fit/Spec −217 73 20
Lemasle et al. (2014) For Phot 68 56 2 −235 66 36
Skúladóttir et al. (2015) Scl Phot −57 163 7 −157 82 72
Hill et al. (2019) Scl Phot −57 163 7 −158 79 71
Geisler et al. (2005) Scl Phot −191 74 2
Simon et al. (2015) Scl Spec 3 1
Kirby et al. (2010) Scl Fit/Spec −45 1 −100 87 6
Kirby et al. (2013) Scl Fit/Spec −41 80 4 −100 226 44
Kirby et al. (2010) Sex Fit/Spec −172 1
Kirby et al. (2013) Sex Fit/Spec 205 249 7 58 251 18
Shetrone et al. (2001) Sex Spec −172 1
Sbordone et al. (2007) Sgr Phot −96 114 12
Hansen et al. (2018) Sgr Spec −89 367 2 −130 81 11
Bonifacio et al. (2004) Sgr Phot 26 66 9
Koch et al. (2008) Car Phot −167 1
Norris et al. (2017) Car Phot −50 1 −61 115 9
Fabrizio et al. (2012) Car Phot −110 1 −78 119 17
Lemasle et al. (2012) Car Phot 174 341 4 −112 150 29
Ural et al. (2015) UMi Spec 129 1 −23 21 2
All studies 132 260 62 −119 137 462

Notes. “Method Tlit” indicates the method used in the literature to determine the effective temperature: photometrically (Phot), spectoscopically (Spec), or with fits over spectral regions (Fit).

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