Evans, C. J.C. J.EvansBarbuy, B.B.BarbuyCastilho, B.B.CastilhoSmiljanic, R.R.SmiljanicMelendez, J.J.MelendezJapelj, J.J.JapeljCRISTIANI, StefanoStefanoCRISTIANISnodgrass, C.C.SnodgrassBonifacio, P.P.BonifacioPuech, M.M.PuechQuirrenbach, A.A.Quirrenbach2022-03-282022-03-2820180277-786Xhttp://hdl.handle.net/20.500.12386/31938In the era of Extremely Large Telescopes, the current generation of 8-10m facilities are likely to remain competitive at far-blue visible wavelengths for the foreseeable future. High-efficiency (<20%) observations of the ground UV (300- 400 nm) at medium resolving power (R 20,000) are required to address a number of exciting topics in stellar astrophysics, while also providing new insights in extragalactic science. Anticipating strong demand to better exploit this diagnostic-rich wavelength region, we revisit the science case and instrument requirements previously assembled for the CUBES concept for the Very Large Telescope.STAMPAenConference paper10.1117/12.2312022https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10702/2312022/Revisiting-the-science-case-for-near-UV-spectroscopy-with-the/10.1117/12.2312022.full?SSO=12018SPIE10702E..2EEFIS/05 - ASTRONOMIA E ASTROFISICA