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Star formation histories of z~1 galaxies in LEGA C

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Figure

Table 1. Properties of the FSPS template spectra.
Figure 2.Reconstructed SFH (black) of a synthetic galaxy (green) with S/N = 10 respectively, as explained in Sectionwith precisionThe converged walkers are shown in grey and the upper and lower uncertainties are based on the 16A˚−1 (left) and S/N = 30 ˚A−1
Figure 3. Distributions of M∗,F IT (left), a<MW > (middle) and a<LW > (right) of the LEGA-C sample
Figure 4. Sample of emission line subtracted spectra of 12 LEGA-C galaxies with the best fitting model obtained from combiningthe 12 template spectra using MCMC
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