Data from : The SAMI Galaxy Survey: reconciling strong emission line metallicity diagnostics using metallicity gradients

Full description

We measure the gas-phase metallicity gradients of 248 galaxies selected from Data Release 2 of the SAMI Galaxy Survey. We demonstrate that there are large systematic discrepancies between the metallicity gradients derived using common strong emission line metallicity diagnostics. We determine which pairs of diagnostics have Spearman’s rank coefficients greater than 0.6 and provide linear conversions to allow the accurate comparison of metallicity gradients derived using different strong emission line diagnostics. For galaxies within the mass range 8.5 < log (M/M⊙) < 11.0, we find discrepancies of up to 0.11 dex/Re between seven popular diagnostics in the metallicity gradient–mass relation. We find a suggestion of a break in the metallicity gradient–mass relation, where the slope shifts from negative to positive, occurs between 9.5 < log (M/M⊙) < 10.5 for the seven chosen diagnostics. Applying our conversions to the metallicity gradient–mass relation, we reduce the maximum dispersion from 0.11 dex/Re to 0.02 dex/Re. These conversions provide the most accurate method of converting metallicity gradients when key emission lines are unavailable. We find that diagnostics that share common sets of emission line ratios agree best, and that diagnostics calibrated through the electron temperature provide more consistent results compared to those calibrated through photoionization models.

Notes

External Organisations
ARC Centre of Excellence for All-sky Astrophysics; ARC Centre of Excellence for Astrophysics in Three Dimensions (ASTRO3D); University of New South Wales; Universidad Nacional Autónoma de México; University of Toledo; Macquarie University; University of Sydney; NASA, National Aeronautics & Space Administration (NASA), Armstrong Flight Res Ctr, SOFIA Operat Ctr, USRA; Australian Astronomical Optics; Christ University, Bangalore

Associated Persons
Henry Poetrodjojo (Creator); Lisa J. Kewley (Creator); Sarah M. Sweet (Creator); Sebastian F. Sanchez (Creator); Anne M. Medling (Creator); Ángel R. López-Sánchez (Creator); Sarah Brough (Creator); Jesse Van De Sande (Creator); Sam P. Vaughan (Creator); Samuel N. Richards (Creator); Julia J. Bryant (Creator); Scott M. Croom (Creator); Joss Bland-Hawthorn (Creator); Michael Goodwin (Creator); Jon S. Lawrence (Creator); Matt S. Owers (Creator); Nicholas Scott (Creator)