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Fig. 1.

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1D spectra examples from the parent sample. Back solid line and green shaded region represent the flux and associated error respectively. For each galaxy, we report the emission line features spotted for the identification of the spectroscopic redshift. The position of the Lyα line is also highlighted. MSA ID = 44 and 1374 are Lyα emitters with S/N > 3, while MSA ID = 1023, 397, and 11 117 have no Lyα in emission. We report wavelengths in the rest-frame for clarity.

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