On the 3D structure of the mass, metallicity, and SFR space for SF galaxies
Maritza A. Lara-Lopez, Angel R. Lopez-Sanchez, Andrew M. Hopkins

TL;DR
This paper shows that the complex relationship between star formation rate, metallicity, and stellar mass in star-forming galaxies can be effectively represented as a two-dimensional plane, refining previous models and highlighting calibration limitations.
Contribution
It introduces a new analysis of the 3D SFR-metallicity-mass space, demonstrating it can be reduced to a plane and updating the Fundamental Plane with improved methods.
Findings
The 3D space can be represented by a plane using PCA and regression.
The best-fit plane is a regression of stellar mass on SFR and metallicity.
Empirical metallicity calibrations have limitations, especially at high metallicity.
Abstract
We demonstrate that the space formed by the star-formation rate (SFR), gas-phase metallicity (Z), and stellar mass (M), can be reduced to a plane, as first proposed by Lara-Lopez et al. We study three different approaches to find the best representation of this 3D space, using a principal component analysis, a regression fit, and binning of the data. The PCA shows that this 3D space can be adequately represented in only 2 dimensions, i.e., a plane. We find that the plane that minimises the chi^2 for all variables, and hence provides the best representation of the data, corresponds to a regression fit to the stellar mass as a function of SFR and , M=f(Z,SFR). We find that the distribution resulting from the median values in bins for our data gives the highest chi^2. We also show that the empirical calibrations to the oxygen abundance used to derive the Fundamental Metallicity Relation…
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