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Autor:
Cosentino, Rosario, Hernandez, Marcos, Ventura, Hector, Campana, Sergio, Claudi, Riccardo, Schipani, Pietro, Aliverti, Matteo, Baruffolo, Andrea, Ben-Ami, Sagi, Biondi, Federico, Capasso, Giulio, D'Alessio, Francesco, D'Avanzo, Paolo, Hershko, Ofir, Kuncarayakti, Hanindyo, Landoni, Marco, Munari, Matteo, Pignata, Giuliano, Rubin, Adam, Scuderi, Salvatore, Vitali, Fabrizio, Young, David, Achren, Jani, Duran, Jose Antonio Araiza, Arcav, Iair, Brucalassi, Anna, Bruch, Rachel, Cappellaro, Enrico, Colapietro, Mirko, Della Valle, Massimo, De Pascale, Marco, Di Benedetto, Rosario, D'Orsi, Sergio, Gal-Yam, Avishay, Genoni, Matteo, Kotilainenj, Jari, Causi, Gianluca Li, Marty, Laurent, Mattila, Seppo, Rappaport, Michael, Radhakrishnan, Kalyan, Ricci, Davide, Riva, Marco, Salasnich, Bernardo, Slemer, Alessandra, Smartt, Stephen, Sanchez, Ricardo Zanmar, Stritzinger, Maximilian
SOXS is the new spectrograph for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-2000 nm). In this article, we describe the final design of the visible camera cryos
Externí odkaz:
http://arxiv.org/abs/2209.07155
