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Fig. 17.

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Example of ODHIN de-blending of two close sources MID-7636 (RID-25333), a z = 0.5 star forming galaxy, and MID-6294 (RID-22260), a z = 5.5 Lyα emitter. The separation of the sources is 0.4 arcsec. The top row of panels shows, from left to right: the HST F775W, MUSE white-light, [OIII]5007 Å and Lyα narrow band images (5 × 5 arcsec2 size). The central and bottom panels display the spectra derived from ODHIN (in blue) and ORIGIN extraction (in orange) for each source. Fluxes and observed wavelengths are expressed in units of 10−20 erg s−1 cm−2 Å−1 and Å, respectively.

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