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url: http://adsabs.harvard.edu/abs/2016SPIE.9909E..31F
Viotto, V., J. Farinato, D. Greggio, D. Vassallo, E. Carolo, A. Baruffolo, M. Bergomi, A. Carlotti, M. De Pascale, V. D'Orazi, D. Fantinel, D. Magrin, L. Marafatto, L. Mohr, R. Ragazzoni, B. Salasnich and C. Verinaud: SHARK-NIR system design analysis overview. SPIE, Bellingham, Wash. (2016).
url: http://adsabs.harvard.edu/abs/2016SPIE.9911E..27V
Farinato, J., C. Baffa, A. Baruffolo, M. Bergomi, L. Carbonaro, A. Carlotti, M. Centrone, J. Codona, M. Dima, S. Esposito, D. Fantinel, G. Farisato, W. Gaessler, E. Giallongo, D. Greggio, P. Hinz, F. Lisi, D. Magrin, L. Marafatto, F. Pedichini, E. Pinna, A. Puglisi, R. Ragazzoni, B. Salasnich, M. Stangalini, C. Verinaud and V. Viotto: The NIR arm of SHARK: System for coronagraphy with high-order adaptive optics from R to K bands. In: International Journal of Astrobiology 14, 3, 365-373 (2015).
url: http://cdsads.u-strasbg.fr/abs/2015IJAsB..14..365F
Farinato, J., C. Baffa, A. Baruffolo, M. Bergomi, L. Carbonaro, A. Carlotti, M. Centrone, J. Codona, M. Dima, S. Esposito, D. Fantinel, G. Farisato, W. Gaessler, E. Giallongo, D. Greggio, P. Hinz, F. Lisi, D. Magrin, L. Marafatto, F. Pedichini, E. Pinna, A. Puglisi, R. Ragazzoni, B. Salasnich, M. Stangalini, C. Verinaud and V. Viotto: The NIR arm of SHARK: System for coronagraphy with high-order adaptive optics from R to K bands. In: International Journal of Astrobiology 14, 3, 365-373 (2015).
url: http://cdsads.u-strasbg.fr/abs/2015IJAsB..14..365F
Conrad, A. R., C. Arcidiacono, H. Baumeister, M. Bergomi, T. Bertram, J. Berwein, F. Briegel, J. Farinato, T. Herbst, R. Hofferbert, F. Kittmann, M. Kürster, D. Kopon, L. Marafatto, M. Norris, R. Ragazzoni and V. Viotto: Acquiring multiple stars with the LINC-NIRVANA Pathfinder. SPIE, Bellingham, Wash. (2014).
url: http://adsabs.harvard.edu/abs/2014SPIE.9149E..1OC
Radhakrishnan Santhakumari, K. K., L. Marafatto, M. Bergomi, V. Viotto, J. Farinato, R. Ragazzoni, T. Herbst, T. Bertram, M. Dima, P. Bizenberger, F. Briegel, F. Kittmann, L. Mohr and D. Magrin: Ground layer correction: the heart of LINC-NIRVANA. SPIE, Bellingham, Wash. (2014).
url: http://cdsads.u-strasbg.fr/abs/2014SPIE.9148E..2RR
Kopon, D., A. Conrad, C. Arcidiacono, T. Herbst, V. Viotto, J. Farinato, M. Bergomi, R. Ragazzoni, L. Marafatto, H. Baumeister, T. Bertram, J. Berwein, F. Briegel, R. Hofferbert, F. Kittmann, M. Kürster, L. Mohr and K. Radhakrishnan: Pathfinder first light: alignment, calibration, and commissioning of the LINC-NIRVANA ground-layer adaptive optics subsystem. SPIE, Bellingham, Wash. (2014).
url: http://adsabs.harvard.edu/abs/2014SPIE.9148E..28K
Farinato, J., F. Pedichini, E. Pinna, F. Baciotti, C. Baffa, A. Baruffolo, M. Bergomi, P. Bruno, E. Cappellaro, L. Carbonaro, A. Carlotti, M. Centrone, L. Close, J. Codona, S. Desidera, M. Dima, S. Esposito, D. Fantinel, G. Farisato, A. Fontana, W. Gaessler, E. Giallongo, R. Gratton, D. Greggio, J. C. Guerra, O. Guyon, P. Hinz, F. Leone, F. Lisi, D. Magrin, L. Marafatto, M. Munari, I. Pagano, A. Puglisi, R. Ragazzoni, B. Salasnich, E. Sani, S. Scuderi, M. Stangalini, V. Testa, C. Verinaud and V. Viotto: SHARK (System for coronagraphy with High order Adaptive optics from R to K band): a proposal for the LBT 2nd generation instrumentation. SPIE, Bellingham, Wash. (2014).
url: http://cdsads.u-strasbg.fr/abs/2014SPIE.9147E..7JF
Conrad, A. R., C. Arcidiacono, H. Baumeister, M. Bergomi, T. Bertram, J. Berwein, F. Briegel, J. Farinato, T. Herbst, R. Hofferbert, F. Kittmann, M. Kürster, D. Kopon, L. Marafatto, M. Norris, R. Ragazzoni and V. Viotto: Acquiring multiple stars with the LINC-NIRVANA Pathfinder. SPIE, Bellingham, Wash. (2014).
url: http://adsabs.harvard.edu/abs/2014SPIE.9149E..1OC
Radhakrishnan Santhakumari, K. K., L. Marafatto, M. Bergomi, V. Viotto, J. Farinato, R. Ragazzoni, T. Herbst, T. Bertram, M. Dima, P. Bizenberger, F. Briegel, F. Kittmann, L. Mohr and D. Magrin: Ground layer correction: the heart of LINC-NIRVANA. SPIE, Bellingham, Wash. (2014).
url: http://cdsads.u-strasbg.fr/abs/2014SPIE.9148E..2RR
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