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  5. CUBES: a UV spectrograph for the future
 

CUBES: a UV spectrograph for the future

Journal
MEMORIE DELLA SOCIETA ASTRONOMICA ITALIANA  
Date Issued
2023
Author(s)
COVINO, Stefano  
•
CRISTIANI, Stefano  
•
ALCALA', JUAN MANUEL  
•
Alencar, S. H. P.
•
Balashev, S. A.
•
Barbuy, B.
•
Bastian, N.
•
Battino, U.
•
Bissell, L.
•
Bristow, P.
•
Calcines, A.
•
CALDERONE, GIORGIO  
•
Cambianica, P.
•
CARINI, Roberta  
•
Carter, B.
•
CASSISI, Santi  
•
Castilho, B. V.
•
CESCUTTI, Gabriele  
•
Christlieb, N.
•
CIRAMI, Roberto  
•
Conzelmann, R.
•
CORETTI, Igor  
•
Cooke, R.
•
CREMONESE, Gabriele  
•
Cunha, K.
•
CUPANI, Guido  
•
da Silva, A. R.
•
D'Auria, D.
•
DE CAPRIO, VINCENZO  
•
De Cia, A.
•
Dekker, H.
•
D'Elia, V.
•
De Silva, G.
•
Diaz, M.
•
DI MARCANTONIO, Paolo  
•
D'ODORICO, Valentina  
•
Ernandes, H.
•
Evans, C.
•
Fitzsimmons, A.
•
FRANCHINI, Mariagrazia  
•
Gänsicke, B.
•
GENONI, Matteo  
•
Giribaldi, R. E.
•
Gneiding, C.
•
GRAZIAN, Andrea  
•
Hansen, C. J.
•
Hopgood, J.
•
Izzo, L.
•
Kosmalski, J.
•
La Forgia, F.
•
La Penna, P.
•
LANDONI, Marco  
•
Lazzarin, M.
•
Lunney, D.
•
Maciel, W.
•
Marcolino, W.
•
MARCONI, Marcella  
•
MIGLIORINI, Alessandra  
•
Miller, C.
•
Modigliani, A.
•
Noterdaeme, P.
•
OGGIONI, Luca  
•
Opitom, C.
•
PARIANI, Giorgio  
•
Pilecki, B.
•
PIRANOMONTE, Silvia  
•
Quirrenbach, A.
•
Redaelli, E. M. A.
•
Pereira, C. B.
•
RANDICH, Maria Sofia  
•
Rossi, S.
•
Sanchez-Janssen, R.
•
Schoeller, M.
•
Seifert, W.
•
Smiljanic, R.
•
Snodgrass, C.
•
Squalli, O.
•
Stilz, I.
•
Stürmer, J.
•
Trost, A.
•
VANZELLA, Eros  
•
VENTURA, Paolo  
•
Verducci, O.
•
Waring, C.
•
Watson, S.
•
Wells, M.
•
Wright, D.
•
Zafar, T.
•
ZANUTTA, Alessio  
•
Zins., G.
DOI
10.36116/MEMSAIT_94N2.2023.281
Abstract
In spite of the advent of extremely large telescopes in the UV/optical/NIR range, the current generation of 8-10m facilities is likely to remain competitive at ground- UV wavelengths for the foreseeable future. The Cassegrain U-Band E cient Spectrograph (CUBES) has been designed to provide high-e ciency (> 40%) observations in the near UV (305-400 nm requirement, 300-420 nm goal) at a spectral resolving power of R > 20,000, although a lower-resolution, sky-limited mode of R ∼ 7,000 is also planned. CUBES will o er new possibilities in many fields of astrophysics, providing access to key lines of stellar spectra: a tremendous diversity of iron-peak and heavy elements, lighter elements as well as Balmer lines and the Balmer jump. The UV range is also critical in extragalactic studies: the circumgalactic medium of distant galaxies, the contribution of different types of sources to the cosmic UV background, the measurement of H2 and primordial Deuterium in a regime of relatively transparent intergalactic medium, and follow-up of explosive transients. The CUBES project has entered Phase B, dedicated to detailed design and construction. First science operations are planned for 2028.
Coverage
HACK100
All editors
Bonifacio, P.; Molaro, P.
Volume
94
Start page
281
Uri
http://hdl.handle.net/20.500.12386/35389
Url
https://www.memsait.it/volumi/MemSAIT-vol94-n2-2023.php
Issn Identifier
0037-8720
Ads BibCode
2023MmSAI..94b.281C
Rights
open.access
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