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Please use this identifier to cite or link to this item: http://hdl.handle.net/1843/60405
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dc.creatorChris Evanspt_BR
dc.creatorNate Bastianpt_BR
dc.creatorUmberto Battinopt_BR
dc.creatorPamela Cambianicapt_BR
dc.creatorRoberta Carinipt_BR
dc.creatorBrad Carterpt_BR
dc.creatorSanti Cassisipt_BR
dc.creatorBruno Vaz Castilhopt_BR
dc.creatorNorbert Christliebpt_BR
dc.creatorRyan Cookept_BR
dc.creatorStefano Covinopt_BR
dc.creatorStefano Cristianipt_BR
dc.creatorGabriele Cremonesept_BR
dc.creatorKatia Cunhapt_BR
dc.creatorAndré R. da Silvapt_BR
dc.creatorValerio D'Eliapt_BR
dc.creatorAnnalisa de Ciapt_BR
dc.creatorGayandhi de Silvapt_BR
dc.creatorMarcos Diazpt_BR
dc.creatorPaolo di Marcantoniopt_BR
dc.creatorHeitor Ernandespt_BR
dc.creatorAlan Fitzsimmonspt_BR
dc.creatorCyrielle Opitompt_BR
dc.creatorMariagrazia Franchinipt_BR
dc.creatorBoris T. Gänsickept_BR
dc.creatorMatteo Genonipt_BR
dc.creatorRiano E. Giribaldipt_BR
dc.creatorAndrea Grazianpt_BR
dc.creatorCamilla Juul Hansenpt_BR
dc.creatorFiorangela La Forgiapt_BR
dc.creatorMonica Lazzarinpt_BR
dc.creatorWagner Marcolinopt_BR
dc.creatorMarcella Marconipt_BR
dc.creatorGabriele Cescuttipt_BR
dc.creatorAlessandra Migliorinipt_BR
dc.creatorPasquier Noterdaemept_BR
dc.creatorClaudio Pereirapt_BR
dc.creatorBogumil Pileckipt_BR
dc.creatorAndreas Quirrenbachpt_BR
dc.creatorSofia Randichpt_BR
dc.creatorSilvia Rossipt_BR
dc.creatorRodolfo Smiljanicpt_BR
dc.creatorColin Snodgrasspt_BR
dc.creatorJulian Stürmerpt_BR
dc.creatorValentina D'Odoricopt_BR
dc.creatorAndrea Trostpt_BR
dc.creatorEros Vanzellapt_BR
dc.creatorPaolo Venturapt_BR
dc.creatorDuncan Wrightpt_BR
dc.creatorTayyaba Zafarpt_BR
dc.creatorJuan Manuel Alcalápt_BR
dc.creatorSilvia Helena Paixao Alencarpt_BR
dc.creatorSergei Balashevpt_BR
dc.creatorBeatriz Barbuypt_BR
dc.date.accessioned2023-10-31T21:40:19Z-
dc.date.available2023-10-31T21:40:19Z-
dc.date.issued2022-10-01-
dc.citation.volume1pt_BR
dc.citation.issue55pt_BR
dc.citation.spage1pt_BR
dc.citation.epage57pt_BR
dc.identifier.doihttps://doi.org/10.1007/s10686-022-09864-7pt_BR
dc.identifier.issn1572-9508pt_BR
dc.identifier.urihttp://hdl.handle.net/1843/60405-
dc.description.resumoWe introduce the scientifc motivations for the development of the Cassegrain U-Band Efcient Spectrograph (CUBES) that is now in construction for the Very Large Telescope. The assembled cases span a broad range of contemporary topics across Solar System, Galactic and extragalactic astronomy, where observations are limited by the performance of current ground-based spectrographs shortwards of 400 nm. A brief background to each case is presented and specifc technical requirements on the instrument design that fow-down from each case are identifed. These were used as inputs to the CUBES design, that will provide a factor of ten gain in efciency for stronomical spectroscopy over 300-405 nm, at resolving powers of R ∼ 24,000 and ∼7,000. We include performance estimates that demonstrate the ability of CUBES to observe sources that are up to three magnitudes fainter than currently possible at ground-ultraviolet wavelengths, and we place its predicted performance in the context of existing facillities.pt_BR
dc.format.mimetypepdfpt_BR
dc.languageengpt_BR
dc.publisherUniversidade Federal de Minas Geraispt_BR
dc.publisher.countryBrasilpt_BR
dc.publisher.departmentICX - DEPARTAMENTO DE FÍSICApt_BR
dc.publisher.initialsUFMGpt_BR
dc.relation.ispartofExperimental Astronomy: Astrophysical Instrumentation and Methodspt_BR
dc.rightsAcesso Abertopt_BR
dc.subjectInstrumentation: spectrographspt_BR
dc.subjectCometspt_BR
dc.subjectStarspt_BR
dc.subjectGalaxiespt_BR
dc.subjectTransientspt_BR
dc.subject.otherAstronomia - instrumentospt_BR
dc.subject.otherEspectroscopia astronômicapt_BR
dc.titleThe CUBES science casept_BR
dc.typeArtigo de Periódicopt_BR
dc.url.externahttps://link.springer.com/article/10.1007/s10686-022-09864-7pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-5171-8376pt_BR
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