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The First Empirical Calibration of the Mid-infrared Abundance Diagnostic Ne23 with JWST

  • Authors: Noah S. J. Rogers, Evan D. Skillman, Danielle A. Berg, Karla Z. Arellano-Córdova, Richard W. Pogge, Alessandra Aloisi, Leslie K. Hunt, Anne E. Jaskot, Matilde Mingozzi, Ryan J. Rickards Vaught, Karin M. Sandstrom, O. Grace Telford, Macarena G. del Valle-Espinosa

Noah S. J. Rogers et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Direct 12+log(O/H) vs. Ne23 measured in the CHAOS H II regions (green diamonds) and low-Z nebulae (purple circles, upper limit represented with a black arrow). In most cases, the uncertainties on the points are smaller than the sizes of the symbols. The linear relation derived from the CHAOS H II regions is plotted as a dashed orange line, which describes the O/H–Ne23 trends at 12+log(O/H) ≳ 7.69 dex (10% solar O/H). A cubic function (solid red) accurately fits O/H at all Ne23, and the red shaded area represents the 16th and 84th percentiles of the resampled fit. The cubic function is offset ∼0.2 dex lower than photoionization model predictions (solid blue; J. A. Fernández-Ontiveros et al. 2021). The lower panel plots the difference between the measured and predicted 12+log(O/H), where the standard deviation is 0.06 dex. Each point is color coded by the [Ne III]/[Ne II] ratio, and no correlation between this ionization tracer and δ(O/H) is detected. These data reveal that Ne23 is a strong predictor of metallicity over 1.5 dex in 12+log(O/H).

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