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Table B.2

Overview of the sample stars with photometric Teff and log g determinations and details regarding the corresponding analysis.

Type of stars # of stars Photom method Type of models Codes vmic indicator measurement error ΔTeff/Δlog gvmic References
O9-B2 V 22 [M3a] LTE/nLTE ATLAS9/DETAL/SURFACE O II ±1.20/±0.10/±1.5 DCB99, D01
B2-B3 IV/III 4 [M3a] LTE ATLAS9/WIDTH9 O II ±1.000.203.0 Smartt et al. (2002)
B2-A1 V/III 45 [M2] LTE ATLAS9 .... ±0.400.091.0 FM05
A5-G2 V/III/Ib 172 [M2] LTE ATLAS9(a)/SPECTRUM .... ±0.080.100.5 GGH01
A0-A8 V/III 46 [M1] LTE ATLAS9(b) O Id ±0.300.300.3 Takeda et al. (2008)
AF V/IV 67 [M1] LTE ATLAS9(b) Fe II/Mg II ±0.12/±0.20/±1.0 G08a, G08b, G10
AFG I/II 63 [M1] LTE ATLAS9 Fe II ±0.12/±0.12/±0.5 L10, L15
FGK V 158 [M3b] LTE MARCS/MOOG Fe I ±0.100.10/.... Luck (2018a)
FGK V 106 [M3a] LTE SAM12/WIOTA6(c) Fe I/II ..../±bf 0.12/±0.2 Ivanyuk et al. (2017)
RGs 35 [M3b] LTE MARCS//MOOG Fe Id/Fe II ±0.260.12/.... Wang et al. (2017)

Notes. ΔTeff in kK; Δlog g in dex; Δvmic in km s−1. Bold faced numbers are upper limits.

(a) – M. Lemke’s distribution of ATLAS9. (b) – A modified version of WIDTH9 developed by Takeda (1995); (c) – Specific codes developed by Pavlenko (2003); (d) – NLTE effects taken into account; D01=Daflon et al. (2001); DCB99=Daflon et al. (1999); G08a=Gebran & Monier (2008a); G08b=Gebran & Monier (2008b); G10=Gebran et al. (2010); GGH=Gray et al. (2001); L10=Lyubimkov et al. (2010); L15=Lyubimkov et al. (2015); FM05=Fitzpatrick & Massa (2005)

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