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The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations

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Academic year: 2020

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Table 1. Global properties of the simulated galaxies used to generate the mock data cubes
Figure 2. Composite synthetic broadband images created in the (u, r, and z)-bands using the Lupton et al
Figure 3. Left-hand panel: RGB image of the [O III ]5007, Hα, and [N II ]6584 emission lines for the galaxy C-CS + 1
Table 3. Sizes of the simulated data cubes in the spatial and spectral dimensions (N α , N δ , and N λ ), wavelength range, spectral sampling, and spectral resolution (λ, d λ , and δ λ ) of each instrumental setup, and best-fitting parameters (σ 0 and I 0
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