A re-assessment of strong line metallicity conversions in the machine learning era
Monthly Notices of the Royal Astronomical Society(2021)
摘要
Strong line metallicity calibrations are widely used to determine the gas phase metallicities of individual H II regions and entire galaxies. Over a decade ago, based on the Sloan Digital Sky Survey Data Release 4, Kewley & Ellison published the coefficients of third-order polynomials that can be used to convert between different strong line metallicity calibrations for global galaxy spectra. Here...
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关键词
galaxies: fundamental parameters,galaxies: abundances,methods: data analysis,methods: statistical,methods: observational,methods: numerical
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