Fig. 1
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Kiel diagram showing best-fit effective temperatures and surface gravities for the sample. The shapes represent the best-fit parameters from the GA. The blue squares are the supergiants, the orange triangles the giants and the green circles the dwarf stars. The crosses are literature measurements of the same parameters from Ramírez-Agudelo et al. (2017) (RA17) for (super)giants or Sabín-Sanjulián et al. (2017) (SS17) for dwarfs. Lines are drawn between points to guide the eye between measurements made for the same star from this work and literature studies. These are overplotted against evolutionary tracks from Brott et al. (2011a) at an LMC metallicity of Z = 0.5 Z⊙ and moderate rotation of v sin i ~ 150–200 km s−1. Each evolutionary track is annotated with the input initial stellar mass.
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