Image Details

Choose export citation format:

The Heavy Metal Survey: The Evolution of Stellar Metallicities, Abundance Ratios, and Ages of Massive Quiescent Galaxies since z ∼ 2

  • Authors: Aliza G. Beverage, Mariska Kriek, Katherine A. Suess, Charlie Conroy, Sedona H. Price, Guillermo Barro, Rachel Bezanson, Marijn Franx, Brian Lorenz, Yilun Ma, Lamiya A. Mowla, Imad Pasha, Pieter van Dokkum, Daniel R. Weisz

Aliza G. Beverage et al 2024 The Astrophysical Journal 966 .

  • Provider: AAS Journals

Caption: Figure 9.

Results from the parameter recovery of mock Heavy Metal spectra. We show systematic offsets in the stellar population fitting code as a function of S/N for four key parameters. At each S/N, we generate 20 mock spectra and fit their elemental abundances and ages following the procedure in Section 2. The black rectangles represent the median offset between the simulated and best-fit values for the 20 realizations. The blue error bars represent the 16th and 84th percentiles of the best-fit values for the 20 realizations. The red error bars show the typical uncertainties on a single realization. The gray tick marks at the bottom of each panel show the true S/N of the individual Heavy Metal spectra. For the typical Heavy Metal galaxy, the systematic offsets are ≈−0.05 dex for [Fe/H] and [Mg/Fe] and ≈0.05 dex for log Age.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse