M. Cirasuolo, O. González, P. Rees, I. Bryson, A. Fairley, W. Taylor, J. Afonso, S. Lilly, C. Evans, H. Flores, R. Maiolino, E. Oliva, S. Paltani, L. Vanzi, M. Abreu, J. Amans, D. Atkinson, S. Beard, C. Béchet, A. Belfiore, M. Black, D. Boettger, S. Brierley, D. Buscher, A. Cabral, M. Carollo, W. Cochrane, J. Coelho, M. Colling, R. Conzelmann, F. D'Alessio, Louise Dauvin, G. Davidson, G. Fasola, D. Ferruzzi, M. Fisher, M. Flores, B. Garilli, A. Gargiulo, J. Gaudemard, I. Guinouard, P. Gutierrez, R. Haigron, C. Haniff, D. Ives, O. Iwert, D. King, Suzanne Kovacz, P. Laporte, David W. Lee, G. Causi, Yerko Luco, A. MacLeod, C. Maire, Basile-Thierry Melse, A. Oliveira, L. Origlia, I. Parry, F. Pedichini, R. Piazzesi, F. Reix, M. Rodrigues, F. Rojas, F. Royer, P. Santos, R. Schnell, T. Shen, M. Sordet, J. Strachan, Xaiowei Sun, G. Tait, A. Tozzi, S. Tulloch, Lauren Von Dran, C. Waring, S. Watson, B. Woodward, Yanbin Yang
{"title":"新月:新VLT的多目标摄谱仪正在进行的建设的更新","authors":"M. Cirasuolo, O. González, P. Rees, I. Bryson, A. Fairley, W. Taylor, J. Afonso, S. Lilly, C. Evans, H. Flores, R. Maiolino, E. Oliva, S. Paltani, L. Vanzi, M. Abreu, J. Amans, D. Atkinson, S. Beard, C. Béchet, A. Belfiore, M. Black, D. Boettger, S. Brierley, D. Buscher, A. Cabral, M. Carollo, W. Cochrane, J. Coelho, M. Colling, R. Conzelmann, F. D'Alessio, Louise Dauvin, G. Davidson, G. Fasola, D. Ferruzzi, M. Fisher, M. Flores, B. Garilli, A. Gargiulo, J. Gaudemard, I. Guinouard, P. Gutierrez, R. Haigron, C. Haniff, D. Ives, O. Iwert, D. King, Suzanne Kovacz, P. Laporte, David W. Lee, G. Causi, Yerko Luco, A. MacLeod, C. Maire, Basile-Thierry Melse, A. Oliveira, L. Origlia, I. Parry, F. Pedichini, R. Piazzesi, F. Reix, M. Rodrigues, F. Rojas, F. Royer, P. Santos, R. Schnell, T. Shen, M. Sordet, J. Strachan, Xaiowei Sun, G. Tait, A. Tozzi, S. Tulloch, Lauren Von Dran, C. Waring, S. Watson, B. Woodward, Yanbin Yang","doi":"10.1117/12.2561229","DOIUrl":null,"url":null,"abstract":"The Multi Object Optical and Near-infrared Spectrograph (MOONS) instrument is the next generation multi-object spectrograph for the VLT. This powerful instrument will combine for the first time: the large collecting power of the VLT with a high multipexing capability offered by 1000 optical fibres moved with individual robotic positioners and a novel, very fast spectrograph able to provide both low- and high-resolution spectroscopy simultaneously across the wavelength range 0.64μm - 1.8μm. Such a facility will provide the astronomical community with a powerful, world-leading instrument able to serve a wide range of Galactic, Extragalactic and Cosmological studies. 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Crescent MOONS: an update on the ongoing construction of the new VLT's multi-object spectrograph
The Multi Object Optical and Near-infrared Spectrograph (MOONS) instrument is the next generation multi-object spectrograph for the VLT. This powerful instrument will combine for the first time: the large collecting power of the VLT with a high multipexing capability offered by 1000 optical fibres moved with individual robotic positioners and a novel, very fast spectrograph able to provide both low- and high-resolution spectroscopy simultaneously across the wavelength range 0.64μm - 1.8μm. Such a facility will provide the astronomical community with a powerful, world-leading instrument able to serve a wide range of Galactic, Extragalactic and Cosmological studies. Th final assembly, integration and verification phase of the instrument is now about to start performance testing.
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