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Fig. 6.

image

Examples of PYPLATEFIT spectral fitting, for two sources in our catalogues. Top row shows the case of the bright z = 4.03 galaxy in MACS0940 (Claeyssens et al. 2019) with zconf = 3 and the bottom row a MUSELET-selected galaxy at z = 0.337 and zconf = 2 in the same cluster field (M364). The left panel gives an overview of the spectrum, while the middle and right panels zoom in on specific spectral line fits. The best-fit spectrum and global continuum fit are plotted in red and blue, respectively.

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