A4 Vertaisarvioitu artikkeli konferenssijulkaisussa
Characterisation and assessment of the SOXS Spectrograph UV-VIS Detector System
Tekijät: Cosentino, Rosario; Hernandez, Marcos; Ventura, Hector; Campana, Sergio; Claudi, Riccardo; Schipani, Pietro; Aliverti, Matteo; Asquini, Laura; Baruffolo, Andrea; Battain, Federico; Ben-Ami, Sagi; Bichkovsky, Alex; 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; Afchren, Jani; Araiza-Duran, Jose Antonip; Arcavi, Iair; Brucalassi, Anna; Bruch, Rachel; Cappellaro, Enrico; Colapietro, Mirko; Della Valle, Massimo; Di Benedetto, Rosario; Di Filippo, Simone; D'Orsi, Sergio; Gal-Yam, Avishay; Genoni, Matteo; Kotilainen, Jari; Li Causi, Gianluca; Marty, Laurent; Mattila, Seppo; Rappaport, Michael; Radhakrishnan, Kalyan; Ricci, Davide; Riva, Marco; Salasnich, Bernardo; Savarese, Salvatore; Smartt, Stephen; Sanchez, Ricardo Zanmar; Stritzinger, Maximilian; Accardo, Matteo; Mehrgan, Leander H.; Ives, Derek
Toimittaja: Bryant, JJ; Motohara, K; Vernet, JR
Konferenssin vakiintunut nimi: SPIE Astronomical Telescopes + Instrumentation
Kustantaja: SPIE-INT SOC OPTICAL ENGINEERING
Kustannuspaikka: BELLINGHAM
Julkaisuvuosi: 2024
Journal: Proceedings of SPIE : the International Society for Optical Engineering
Kokoomateoksen nimi: Ground-based and Airborne Instrumentation for Astronomy X
Lehden akronyymi: PROC SPIE
Artikkelin numero: 130962U
Sarjan nimi: Proceedings of SPIE
Vuosikerta: 13096
Sivujen määrä: 9
ISBN: 978-1-5106-7515-5
eISBN: 978-1-5106-7516-2
ISSN: 0277-786X
eISSN: 1996-756X
DOI: https://doi.org/10.1117/12.3019853
Verkko-osoite: https://doi.org/10.1117/12.3019853
Preprintin osoite: https://arxiv.org/abs/2407.17245
The SOXS spectrograph, designed for the ESO NTT telescope, operates in both the optical (UV-VIS: 350-850 nm) and NIR (800-2000 nm) bands. This article provides an overview of the final tests conducted on the UV-VIS camera system using a telescope simulator. It details the system's performance evaluation, including key metrics such as gain, readout noise, and linearity, and highlights the advancements made in the upgraded acquisition system. The testing process, conducted in the Padua laboratory, involved comprehensive simulations of the telescope environment to ensure the results closely resemble those expected at the ESO-NTT telescope. The successful completion of these tests confirms the system's readiness for deployment to Chile, where it will be installed on the NTT telescope, marking a significant milestone in the SOXS project.
