A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
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Large-sample analysis finds Te([N II]) relations have lower dispersion than those for [O II] or [S II], making it a more reliable low-ionization temperature proxy.
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Consistent Gas-Phase Temperatures and Metallicities from UV and Optical Nebular Emission: A Reliable Foundation from z=0 to Cosmic Dawn
A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
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The DESIRED electron temperature relations in star-forming regions of the local Universe
Large-sample analysis finds Te([N II]) relations have lower dispersion than those for [O II] or [S II], making it a more reliable low-ionization temperature proxy.