Figure 7.
![Distribution of the LAMOST–APOGEE training stars in the Teff–log g and [M/H]–[α/M] planes. Values of Teff are those derived with LSP3, while those of log g, [M/H] and [α/M] are from the APOGEE catalogue (Holtzman et al. 2015).](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/464/3/10.1093_mnras_stw2523/4/stw2523fig7.jpeg?Expires=1750625888&Signature=GUwEk2fC7OwBV90pyWfrSKtfO36oGyMqGZ8NIiqlrM-fUtZZwr-Dr61QExtMleD2y6O6ypUpXl7~ZdEZ20wpgvd7RMuHaNDaKPOA8V8trvcu2JSKj00DOhz~cguGtyhYVwqGFGQ1puqmM8KCp1kBSDBPcSXhIErA44KNaIyP1YmLckdAuTqjnBtp4T1KO70DIbm0ONAr8Wlnxc5gpaNX1eh7NX0N4gMZAYbMIj2Z7G-HVF0UxjZcuxBIrCFf-7Km1UkF5BEpwFgv~JG~E21O0dx7y6HnlmayWh62PNO8z52D2EnlUnFjfQexl1kJZTutJ4GVXwJQaPQTqKSFBIkQXQ__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Distribution of the LAMOST–APOGEE training stars in the Teff–log g and [M/H]–[α/M] planes. Values of Teff are those derived with LSP3, while those of log g, [M/H] and [α/M] are from the APOGEE catalogue (Holtzman et al. 2015).
Distribution of the LAMOST–APOGEE training stars in the Teff–log g and [M/H]–[α/M] planes. Values of Teff are those derived with LSP3, while those of log g, [M/H] and [α/M] are from the APOGEE catalogue (Holtzman et al. 2015).
