Correction to Conversions between gas-phase metallicities in MaNGA

Abstract

We present a brief correction to Scudder et al. (2021) due to an error in the O3N2 based metallicity calibrations presented in that work. Conclusions are unchanged, but metallicity values shift by $\sim$0.03 dex, with polynomials for affected conversions shifted by the same amount. We present updated materials here.

arXiv comment4 pages, 3 figures. Supplementary materials available online. Accepted for publication in MNRAS

References in corpus (4)

• [O III]/[N II] as an Abundance Indicator at High Redshift
• The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and Te-based literature data
• New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies
• Conversions between gas-phase metallicities in MaNGA