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Fig. 2.

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Spectra of multiply lensed sources. Blue lines indicate the spectroscopic data and gray regions of variance. Vertical lines show the main spectral features present in each wavelength range. In cases where the continuum is clearly detected, the red line corresponds to the template used to estimate the exact redshift. The small HST cutouts in the top-left region of each panel are 2 arcsec per side.

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