ANDES, the High Resolution Spectrograph for the ELT: Science Case, Baseline Design and Path to Construction
A. Marconi,M. Abreu,V. Adibekyan,V. Alberti,S. Albrecht,J. Alcaniz,M. Aliverti,C. Allende Prieto, J. D. Alvarado Gomez,P. J. Amado,M. Amate,M. I. Andersen,E. Artigau,C. Baker,V. Baldini,A. Balestra,S. A. Barnes,F. Baron,S. C. C. Barros,S. M. Bauer,M. Beaulieu,O. Bellido-Tirado,B. Benneke,T. Bensby, E. A. Bergin,K. Biazzo,A. Bik,J. L. Birkby,N. Blind,I. Boisse,E. Bolmont,M. Bonaglia,X. Bonfils,F. Borsa,A. Brandeker,W. Brandner,C. H. Broeg,M. Brogi,D. Brousseau,A. Brucalassi,J. Brynnel,L. A. Buchhave,D. F. Buscher,A. Cabral,G. Calderone,R. Calvo-Ortega,F. Cantalloube,B. L. Canto Martins,L. Carbonaro,G. Chauvin,B. Chazelas, A. -L. Cheffot,Y. S. Cheng,A. Chiavassa,L. Christensen,R. Cirami,N. J. Cook,R. J. Cooke,I. Coretti,S. Covino,N. Cowan,G. Cresci,S. Cristiani,V. Cunha Parro,G. Cupani,V. D'Odorico,I. de Castro Leao,A. De Cia,J. R. De Medeiros,F. Debras,M. Debus,O. Demangeon,M. Dessauges-Zavadsky,P. Di Marcantonio,F. Dionies,R. Doyon,J. Dunn,D. Ehrenreich,J. P. Faria,C. Feruglio,M. Fisher,A. Fontana,M. Fumagalli,T. Fusco,J. Fynbo,O. Gabella,W. Gaessler,E. Gallo,X. Gao,L. Genolet,M. Genoni,P. Giacobbe,E. Giro,R. S. Goncalves,O. A. Gonzalez,J. I. Gonzalez Hernandez, F. Gracia Temich,M. G. Haehnelt,C. Haniff,A. Hatzes,R. Helled,H. J. Hoeijmakers,P. Huke, A. S. Jaervinen,S. P. Jaervinen,A. Kaminski,A. J. Korn,D. Kouach,G. Kowzan,L. Kreidberg,M. Landoni, A. Lanotte,A. Lavail,J. Li,J. Liske,C. Lovis,S. Lucatello,D. Lunney,M. J. MacIntosh,N. Madhusudhan,L. Magrini,R. Maiolino,L. Malo,A. W. S. Man,T. Marquart, E. L. Marques,C. J. A. P. Martins, A. M. Martins,P. Maslowski,E. Mason,C. A. Mason,R. A. McCracken, P. Mergo,G. Micela,T. Mitchell,P. Molliere,M. A. Monteiro,D. Montgomery,C. Mordasini,J. Morin,A. Mucciarelli,M. T. Murphy,M. N'Diaye,B. Neichel,A. T. Niedzielski,E. Niemczura,L. Nortmann,P. Noterdaeme,N. J. Nunes,L. Oggioni,E. Oliva,H. Onel,L. Origlia,G. Ostlin,E. Palle,P. Papaderos,G. Pariani, J. Penate Castro,F. Pepe,L. Perreault Levasseur,P. Petit,L. Pino, J. Piqueras,A. Pollo,K. Poppenhaeger,A. Quirrenbach,E. Rauscher,R. Rebolo,E. M. A. Redaelli,S. Reffert,D. T. Reid,A. Reiners,P. Richter,M. Riva,S. Rivoire,C. Rodriguez-Lopez,I. U. Roederer,D. Romano,S. Rousseau,J. Rowe,S. Salvadori,N. Sanna,N. C. Santos, P. Santos Diaz,J. Sanz-Forcada,M. Sarajlic,J. -F. Sauvage,S. Schaefer,R. P. Schiavon,T. M. Schmidt,C. Selmi,S. Sivanandam,M. Sordet,R. Sordo,F. Sortino,D. Sosnowska,S. G. Sousa,E. Stempels,K. G. Strassmeier,A. Suarez Mascareno,A. Sulich,X. Sun,N. R. Tanvir, F. Tenegi-Sangines,S. Thibault,S. J. Thompson,A. Tozzi,M. Turbet,P. Vallee,R. Varas,K. A. Venn,J. -P. Veran,A. Verma,M. Viel,G. Wade,C. Waring,M. Weber,J. Weder,B. Wehbe,J. Weingrill,M. Woche,M. Xompero,E. Zackrisson,A. Zanutta,M. R. Zapatero Osorio,M. Zechmeister, J. Zimara
GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY IX（2022）
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ground-based instruments,high resolution spectrographs,infrared spectrographs,extremely large telescopes,exoplanets,stars and planets formation,physics and evolution of stars,physics and evolution of galaxies,cosmology,fundamental physics
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