摘要：Referencestothefiguresinthetextarenotcorrect.Thecorrected figure references along with the respective texts of the original paper are as follows: – Caption of Fig. 5: References to right and left panels are in- verted. The corrected figure caption is: Left panel: comparison of T eff versus spectral type relation as a function of metallicity from this study with Passegger et al. (2018; open triangle) and with Rajpurohit et al. (2013; open circle). Right panel: comparison of T eff determined from this study with Passegger et al. (2018; open triangle) and with Gaidos & Mann (2014; filled square) as function of metallicity. – Corrected text (page 5, right column): In order to explore the effect of stellar properties of M dwarfs, we have compared our results with the behavior of T eff , as a function of spectral type with Rajpurohit et al. (2013) as shown in Fig. 5 (left panel). – Corrected text (page 5, right column): In order to explore further, we compared T eff determination with Gaidos & Mann (2014; hereafter G14) along with Passegger et al. (2018), for the common stars in our sample as shown in Fig 5 (right panel).
关键词：enstars: fundamental parametersstars: low-massstars: atmosphereserrata, addenda
