Pamela Cambianica
at INAF - Osservatorio Astronomico di Padova
SPIE Involvement:
Author
Publications (1)

Proceedings Article | 29 August 2022 Presentation + Paper
S. Cristiani, J. M. Alcalá, S. H. P. Alencar, S. Balashev, N. Bastian, B. Barbuy, U. Battino, A. Calcines , G. Calderone, P. Cambianica, R. Carini, B. Carter, S. Cassisi, B. Castilho, G. Cescutti, N. Christlieb, R. Cirami, I. Coretti, R. Cooke, S. Covino, G. Cremonese, K. Cunha, G. Cupani, A. da Silva, V. De Caprio, A. De Cia, H. Dekker, V. D'Elia, G. de Silva, M. Diaz, P. Di Marcantonio, D. D'Auria, V. D'Odorico, A. Fitzsimmons, H. Ernandes, C. Evans, M. Franchini, M. Genoni, B. Gänsicke, R. E. Giribaldi, C. Gneiding, A. Grazian, C. J. Hansen, F. La Forgia, M. Landoni, M. Lazzarin, D. Lunney, W. Maciel, W. Marcolino, M. Marconi, A. Migliorini, C. Miller, P. Noterdaeme, C. Opitom, G. Pariani, B. Pilecki, S. Piranomonte, A. Quirrenbach, E. M. A. Redaelli, C. Pereira, S. Randich, S. Rossi, R. Sanchez-Janssen, W. Seifert, R. Smiljanic, C. Snodgrass, I. Stilz, J. Stürmer, E. Vanzella, P. Ventura, O. Verducci, C. Waring, S. Watson, M. Wells, D. Wright, T. Zafar, A. Zanutta
Proceedings Volume 12184, 121840A (2022) https://doi.org/10.1117/12.2629990
KEYWORDS: Spectrographs, Stars, Chemical elements, Ultraviolet radiation, Telescopes, Galactic astronomy, Sensors, Astronomy, Signal to noise ratio, Near ultraviolet

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