GREGGIO, LauraLauraGREGGIOGULLIEUSZIK, MARCOMARCOGULLIEUSZIKFalomo, R.R.FalomoFANTINEL, DanielaDanielaFANTINELUSLENGHI, MICHELAMICHELAUSLENGHI2020-07-072020-07-0720161743-9213http://hdl.handle.net/20.500.12386/26373The extraordinary sensitivity and spatial resolution of the future extremely large telescopes will allow us to extensively characterize the photometrical and structural properties of high redshift galaxies in spite of their very small size. With such future facilities it will be possible to derive both accurate photometry and detailed morphology of very distant galaxies that are mandatory to tackle fundamental problems on the processes of galaxy formation and evolution.STAMPAenConference paper10.1017/S17439213150098982-s2.0-84983336584000452773300011https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/properties-of-high-z-galaxies-in-the-elts-era/083A0B99EAC54A8CE3428A31313DBF1D2016IAUS..319...21GFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering