Morphology and SED modelling of high redshift galaxies in deep Fields - PowerPoint PPT Presentation

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Morphology and SED modelling of high redshift galaxies in deep Fields

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Where, When and How did the Hubble sequence of morphological types form? ... Deep ACS images (i , z) of CL1252-2927 (z=1.23). High sensitivity and angular resolution ... – PowerPoint PPT presentation

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